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    Volcanological perspectives on Long Valley, Mammoth Mountain,

    and Mono Craters: several contiguous but discrete systems

    Wes Hildreth*

    U.S. Geological Survey, Volcano Hazards Team, MS-910, Menlo Park, CA 94025, USA

    Abstract

    The volcanic history of the Long Valley region is examined within a framework of six successive (spatially discrete) foci of

    silicic magmatism, each driven by locally concentrated basaltic intrusion of the deep crust in response to extensional unloading

    and decompression melting of the upper mantle. A precaldera dacite field (3.52.5 Ma) northwest of the later site of Long

    Valley and the Glass Mountain locus of >60 high-silica rhyolite vents (2.2 0.79 Ma) northeast of it were spatially and

    temporally independent magmatic foci, both cold in postcaldera time. Shortly before the 760-ka caldera-forming eruption, the

    mantle-driven focus of crustal melting shifted f 20 km westward, abandoning its long-stable position under Glass Mountain

    and energizing instead the central Long Valley system that released 600 km3 of compositionally zoned rhyolitic Bishop Tuff

    (760 ka), followed by f 100 km3 of crystal-poor Early Rhyolite (760650 ka) on the resurgent dome and later by three

    separate 5-unit clusters of varied Moat Rhyolites of small volume (527101 ka). West of the caldera ring-fault zone, a fourth

    focus started upf

    160 ka, producing a 10

    20-km array of at least 35 mafic

    vents that surround the trachydacite/alkalicrhyodacite Mammoth Mountain dome complex at its core. This young 70-vent system lies west of the structural caldera and

    (though it may have locally re-energized the western margin of the mushy moribund Long Valley reservoir) represents a

    thermally and compositionally independent focus. A fifth major discrete focus started up by f 50 ka, 2530 km north of

    Mammoth Mountain, beneath the center of what has become the Mono Craters chain. In the Holocene, this system advanced

    both north and south, producingf 30 dike-fed domes of crystal-poor high-silica rhyolite, some as young as 650 years. The

    nearby chain of mid-to-late Holocene Inyo domes is a fault-influenced zone of mixing where magmas of at least four kinds are

    confluent. The sixth and youngest focus is at Mono Lake, where basalt, dacite, and low-silica rhyolite unrelated to the Mono

    Craters magma reservoir have erupted in the interval 14 to 0.25 ka. A compelling inference is that mantle-driven magmatic foci

    have moved repeatedly, allowing abandoned silicic reservoirs, including the formerly vigorous Long Valley magma chamber, to

    crystallize. A 100-fold decline of intracaldera eruption rate after 650 ka, lack of crystal-poor rhyolite since 300 ka, limited

    volumes of moat rhyolite (most of it crystal-rich), absence of postcaldera mafic volcanism inside the structural caldera (or north

    and south adjacent to it), low thermal gradients inside the caldera, and sourcing of hydrothermal underflow within the western

    array well outside the ring-fault zone all suggest that the Long Valley magma reservoir is moribund.Published by Elsevier B.V.

    Keywords: magmatism; rhyolites; calderas; Long Valley; Mammoth Mountain; volcanic fields

    0377-0273/$ - see front matter. Published by Elsevier B.V.doi:10.1016/j.jvolgeores.2004.05.019

    * Tel.: +1-650-329-5231; fax: +1-650-329-5203.

    E-mail address:[email protected] (W. Hildreth).

    www.elsevier.com/locate/jvolgeores

    Journal of Volcanology and Geothermal Research 136 (2004) 169 198

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    Fig. 1. Regional location map for Long Valley caldera and contemporaneous volcanic fields within and just east of the Sierra Nevada in east-

    central California. Heavy dashed lines enclose main areas with numerous volcanic vents of Pliocene and Quaternary age (50 Ma). Near 36th

    parallel, Coso and Kern Plateau (KP) volcanic fields have both Pliocene and Quaternary vents, while Panamint Valley (PV) field is Pliocene

    only. Near 37th parallel, Kings River (KR) and Saline Range (SR) volcanic fields are Pliocene while Big Pine (BP) field is Quaternary. Near

    38th parallel, a Pliocene volcanic field continuous from San Joaquin River (SJ) to Adobe Hills (AH) has abundant vents for basalt,

    trachyandesite, and K-rich mafic lavas; near its center, silicic magmas of a more restricted region close to Long Valley caldera (hachured

    enclosure) began erupting f 3.5 Ma, continuing to the present, as detailed in the text and subsequent diagrams. Bold solid lines are faults of

    Pliocene-to-Quaternary age, many with both normal and strike slip displacement, representing encroachment of Basin and Range

    transtensional tectonics (contemporaneous with the volcanism) upon the Sierra Nevada (Mesozoic) batholith province. White areas are

    alluvium-filled basins. Main sources for this diagram:Moore and Dodge (1980);Bacon and Duffield (1981);Duffield and Bacon (1981);Novak

    and Bacon (1986);Ross (1970);Gilbert et al. (1968).

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    Fig. 2. Outline map of Long Valley caldera and adjacent Glass Mountain, Mammoth Mountain, and Mono-Inyo systems, adapted fromBailey

    (1989). Shown for the caldera are its topographic margin (dashed), ring-fault zone (RFZ; dotted), and limit of structurally uplifted resurgent dome

    (RD; dash-dot). The caldera moatis the physiographically low, annular region of the caldera floor that surrounds the resurgent dome, separates it

    from the caldera wall, and conceals the structural ring-fault zone. Four sets of intracaldera rhyolitevents (clustered by both age and location) are

    identified in inset. Dome 7403 in NE moat is early postcaldera rhyodacite. Distribution of precaldera Glass Mountain rhyolite lavas and thick

    pyroclastic apron is shown in pink. Mammoth Mountain trachydacite rhyodacite dome complex is in green, and the array of contemporaneous

    mafic vents around it is patterned grey; the numerous vents are located in Fig. 5.For Mono-Inyo chain, more than 30 rhyolite vents are exposed;

    all but a few are Holocene lava domesthe youngest toward the north and south ends. Place name abbreviations: CM = Crater Mtn;

    DC = Deadman Creek dome; DM = Deer Mtn dome; EQD= Earthquake dome; GC = Glass Creek dome; IC = Inyo Craters (phreatic); JLB = June

    Lake basalt vent; LM = Lookout Mtn; ML= Mammoth Lakes downtown; NC = North Coulee; OD = Obsidian Dome; PB = Punch Bowl;

    PC = Panum Crater; SC = South Coulee; WB = Wilson Butte. Selected faults (after Bailey, 1989) named: ACF= Alpers Canyon fault;

    BMF = Black Mountain fault; FLF = Fern Lake fault; HCF = Hilton Creek fault; HSF = Hartley Springs fault; SLF= Silver Lake fault.

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    crystal-poor; a dozen have 68% phenocrysts, but the

    great majority have 0 5%. Phenocryst abundances,

    species, and compositions resemble those of the

    evolved, first-erupted part of the zoned Bishop Tuff,most units having quartz, sanidine, plagioclase, bio-

    tite, allanite, zircon, apatite, and FeTi oxides. The

    means of generating and sustaining crystal-poor high-

    silica rhyolite for 1.4 Myr are addressed below in

    Section 7.

    3. Climactic eruption and caldera formation

    The caldera-forming eruption of the Bishop Tuff at

    760 ka began as a plinian outburst along or near the

    Hilton Creek fault in the south-central part of what

    soon became the caldera (Hildreth and Mahood,

    1986). The roof of the growing chamber, then about

    5 km deep (Wallace et al., 1999), ultimately failedcatastrophically, releasing f 600 km3 of gas-rich

    rhyolitic magma, compositionally and thermally

    zoned (Hildreth, 1979), i n a virtually continuous

    eruption about 6 days long (Wilson and Hildreth,

    1997), thereby permitting 23 km subsidence of the

    roof, creating the caldera. About half the Bishop Tuff

    volume was emplaced radially as a set of sectorially

    distributed ignimbrite outflow sheets along with con-

    current plinian and coignimbrite fallout. The other

    half ponded inside the subsiding caldera, where

    welded intracaldera ignimbrite is as thick as 1500 m

    Fig. 3. Postcaldera Long Valley rhyolites, simplified from Bailey (1989).Estimated position of main ring-fault zone is 1 to 5 km inboard of

    topographic margin, which receded by syncollapse landsliding and subsequent erosion. Early Rhyolite (760650 ka) lavas in red and tuffs in

    yellow are cut by numerous faults associated with structural uplift. Black stars indicate 13 Early Rhyolite vents exposed (as well as vents for

    younger rhyolites). Three clusters of Moat Rhyolite lavas crop out in north (527481 ka, orange), southeast (362288 ka, green), and west

    (161101 ka, blue); all are crystal-rich except three (of the five) units in the southeastern cluster, which are phenocryst-poor rhyolite lavas

    (distinguished in unpatterned pale green). Arrows generalize lava flow directions. Place name abbreviations: CD = Casa Diablo geothermal

    plant; DCD = Dry Creek dome; DM = Deer Mtn; GD = Gilbert Dome; HCF = Hot Creek flow; LM = Lookout Mtn; MK = Mammoth Knolls (two

    domes); ND = North dome; Ski = Mammoth Mtn ski complex; WMC = West Moat Coulee. Drillholes mentioned in text are: LVEW= Long

    Valley Exploratory Well; SR = Shady Rest; others are named as designated on mapCP-1, M-1, PLV-1, PLV-2, 44-16, 66-29, and Inyo-4.

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    and was subsequently buried by 500 800 m of

    postcaldera rhyolite tuffs, lavas, and sedimentary fill

    (Bailey, 1989). Pumice clasts in the Bishop Tuff are

    zoned from 1 to 25 wt.% phenocrysts and define acompositional continuum in the range 7873% SiO2and 2600 ppm Ba (Hildreth, 1979). The main suite

    of white pumice is accompanied by a sparse popula-

    tion of crystal-poor grey pumice that extends the

    range to 65% SiO2 and to 1350 ppm Ba (Hildreth

    and Wilson, in review).

    The 1732-km depression called Long Valley

    caldera owes its dimensions and the physiography of

    its walls to large-scale syneruptive slumping (cf. Lip-

    man, 1997) and to subsequent secular erosion. As

    inferred from gravity, drillholes, and vent distribution

    (Kane et al., 1976; Carle, 1988; Suemnicht and Varga,

    1988; Bailey, 1989), the ring-fault zone(Figs. 2, 3)

    outlining the area of steep structural collapse of the

    cauldron (roof) block into the magma reservoir

    encloses a subsided oval 12 22 km (f 220 km2),

    roughly 55% of the 400-km2 floor of the topographic-

    hydrographic basin conventionally portrayed as Long

    Valley caldera. The magma chamber, of course, had to

    be somewhat wider than the roof plate that sank into

    it. Nonetheless, clarity in definition of the structural

    caldera can help avoid misleading conceptualizations.

    For example, the Inyo rhyolites are commonly said tohave invaded the caldera 650 years ago and Mammoth

    Mountain is said to straddle the caldera rim. In reality,

    both are extracaldera volcanoes, compositionally and

    spatially independent of the Long Valley reservoir

    (see Sections 5, 6 below).

    Seismic refraction profiles (Hill, 1976; Hill et al.,

    1985) and gravity models (Kane et al., 1976; Carle,

    1988) indicate that the caldera fill thickens substan-

    tially toward the north and east, as confirmed in

    drillholes that show the intracaldera Bishop Tuff

    thickening from 0.9 to 1.2 km centrally to >1.4 km

    in the eastern third of the caldera (Bailey, 1989). What

    fractions of the deepening may reflect precalderatopography, differential magma withdrawal, or tilting

    of the cauldron block during collapse remain uncer-

    tain. The Hilton Creek fault (Fig. 2, where the caldera-

    forming eruption began) clearly had several hundred

    meters of NE-facing precaldera relief, and where the

    caldera center is now, a north-sloping ramp (Bailey,

    1989)probably separated the en-echelon Hilton Creek

    and Hartley Springs faults(Fig. 2).Greater subsidence

    in the north and east is also consistent with strati-

    graphic and petrological evidence that the final erup-

    tive packages of the Bishop Tuff, which preferentially

    flowed toward those sectors, were withdrawn from

    deeper, hotter levels of the magma reservoir(Hildreth,

    1979; Hildreth and Mahood, 1986; Wilson and Hil-

    dreth, 1997; Wallace et al., 1999; Hildreth and Wil-

    son, in review).

    4. Postcaldera eruptive history of Long Valley

    proper

    Compositions of postcollapse eruptive units (750

    to 100 ka) that vented inside or near the calderas ring-fault zone(Fig. 3)are consistent with derivation from

    a reorganized, convectively mixed, and thermally

    restructured Long Valley magma reservoir. Composi-

    tions of silicic units farther west are not. The post-

    caldera units of Long Valley compositional affinity

    (Fig. 4) are (1) rhyodacite Dome 7403, (2) the

    voluminous crystal-poor Early Rhyolites, and (3)

    three sets of Moat Rhyolites (Bailey, 1989)the

    North-central rhyolite chain, the Southeastern rhyolite

    Fig. 4. Compositional contrasts between Long Valley and Mammoth suites. Symbols in inset are for eruptive units discussed in text. LateBishop

    Tuff is the set ofIg2ash-flow packages (ofWilson and Hildreth, 1997), representing magma that issued from the zoned reservoir on the final 2

    days of the 6-day-long caldera-forming eruption. Early Bishop Tuff (EBT), representing the first three quarters of the 600 km 3 of magma

    withdrawn in that eruption, is more homogeneous and barely distinguishable from high-silica rhyolite products of precaldera Glass Mountain

    (GM) and of (largely Holocene) Mono Craters (MC), as grouped in the small shaded fields. (a) Total alkalies vs. SiO 2 (wt.%), showing

    Mammoth Mountain, two sets of western dacites, and crystal-poor Inyo-fp magmas to be more alkalic than the Long Valley suite, which

    includes Bishop Tuff, Early and Moat Rhyolites, and most crystal-rich Inyo-cp magmas. (b) Zr vs. Ba (ppm) for same samples as in top panel,

    showing relative Zr enrichment of Mammoth suite. West Moat Rhyolites plot in two groups, the higher Zr+ Ba (lower SiO2) group representing

    West Moat Coulee and Deer Mountain(Fig. 3).SE Moat Rhyolites also fall in two groups (Fig. 3),the crystal-rich lavas having f 75.5% SiO2and the crystal-poor ones f 76%. The three Inyo-other domes, which predate the 650-year-old eruption, are labelled: ND =North Deadman

    Dome (46 ka);WB = Wilson Butte (1.3 ka); CD = tiny Cratered Dome(post-WB). Data from Hildreth and Wilson (in prep.), Cousens (1996),

    Heumann (1999), Sampson and Cameron (1987),Bailey (1978; 2004),Metz and Mahood (1991),Kelleher and Cameron (1990).

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    cluster, and the West Moat rhyolites. The caldera

    moat is aphysiographicterm for the annular trough

    in resurgent calderas (Smith and Bailey, 1968) that

    separates the central structural uplift from the calderawall; typically the site of postcaldera sedimentation

    and ring-fracture eruptions, the moat conceals and is

    broader than the structural zone of caldera ring faults.

    4.1. Rhyodacite Dome 7403

    In the NE corner of the caldera floor, a small

    rhyodacite lava dome stands alone at the foot of the

    Glass Mountain scarp (Figs. 2, 3). Only 110 m high

    and f 0.01 km3 in volume, this glassy, columnar

    dome, subcircular in plan, is not a downfaulted

    precaldera mass but an unequivocally postcaldera

    eruptive unit.Bailey (1989)suggested that its slender

    glassy columns reflect eruption into a Pleistocene

    intracaldera lake. The dome is compositionally homo-

    geneous (67.8% SiO2with 1550 ppm Ba and 820 ppm

    Sr) but unique in being the only non-rhyolite post-

    caldera eruptive unit from the Long Valley reservoir.

    Rich in small euhedral plagioclase and hornblende

    phenocrysts, it also contrasts with Glass Mountain,

    Bishop Tuff, and early postcaldera rhyolites (Section

    4.2) in having hornblende (instead of biotite or

    pyroxene) as the mafic silicate phase. The lava iscompositionally somewhat like rare dacite pumice

    ejected toward the end of the Bishop Tuff eruption

    (Fig. 4), probably withdrawn from some depth be-

    neath the rhyolite reservoir.

    An attempt was made to determine its age by40Ar/39Ar dating its clean euhedral plagioclase. Al-

    though it contains no obvious xenocrysts, excess Ar

    was indicated by an erratic incremental-fusion spec-

    trum. A few accordant steps in the middle of the Ar-

    release spectrum suggest an early postcaldera age. An

    attempt to date its tiny acicular hornblende euhedra isunderway.

    4.2. Early Rhyolite (ER)

    WhatBailey et al. (1976)termed theEarly Rhyolite

    (Fig. 3) consists of f 100 km3 of fairly uniform,

    phenocryst-poor rhyolite (74 75% SiO2) that erupted

    during the 100,000-year interval following caldera

    collapse. This enormous volume, thicker than 600

    m, is as great as that of precaldera Glass Mountain

    and an order of magnitude greater than the total of all

    subsequent Long Valley rhyolites erupted in the last

    half-million years. Released in scores of separate

    eruptions from at least 13 exposed vents (Bailey,1989), the Early Rhyolite (ER) includes at least 14

    exposed lava flows (and domes), several more inter-

    sected by drilling, and a predominance of varied tuffs

    (fallout and pyroclastic-flow deposits, nonwelded,

    welded, and reworked) that make up about three

    quarters of the ER assemblage. Eight lava flows (but

    no tuffs) have been KAr dated (Mankinen et al.,

    1986), ranging from 751F16 ka to 652F 14 ka.The

    ER extends far beyond its outcrop area (Fig. 3), as

    documented in numerous wells (Suemnicht and

    Varga, 1988; Bailey, 1989). At least 622-m thick near

    its center of outcrop, the ER assemblage is still >350

    m thick where deeply buried in the SE moat and 230-

    to 537-m thick in wells in the west moat.

    Because no correlative layers of distal ash are

    reported outside Long Valley, it seems likely that

    individual eruptions of ER tephra, though numerous,

    were subplinian and modest in volume. This might be

    interpreted to mean that the residual rhyolite magma

    had been relatively depleted in volatiles during the

    caldera-forming eruption, but on the other hand, the

    observation that three quarters of the ER is pyroclastic

    and nearly aphyric indicates that the ER magma waswater-rich. Perhaps, the abundance of medium-scale

    ER eruptions reflected relative ease of magma escape

    through the downfaulted and broken roof plate, there-

    by aborting by frequent eruptive release (and perhaps

    also by passive degassing) any postcaldera recurrence

    of severe gas overpressure.

    Compositions of ER are similar in most respects to

    the last-erupted part of the zoned Bishop Tuff, but for

    a few elements (e.g., Zr and Ba) ER extends the range

    of Bishop zoning(Fig. 4).Phenocryst contents of ER

    are low, only 03%, compared to 1525% in thedirectly preceding, last-erupted part of the Bishop

    Tuff. The dominating minerals in the Bishop Tuff,

    sanidine and quartz, are absent in ER, and the sparse

    crystals present are all new, euhedral, and unresorbed.

    These include plagioclase, orthopyroxene, Fe Ti

    oxides, and (in some units) rare biotite, as well as

    traces of apatite, zircon, and pyrrhotite(Bailey, 1978,

    1989). The contrast in crystal content between late

    Bishop Tuff and (compositionally similar) postcol-

    lapse ER might reflect (1) wholesale resorption of

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    crystals in unerupted rhyolite magma during convec-

    tive reorganization of the postcollapse reservoir, ow-

    ing to heating by (and limited mixing with) hotter

    dacitic or mafic magma drawn up from deeper levels;or (2) pressure-release melting of the crystals in

    rhyolite magma that convectively rose several kilo-

    meters to replace the topmost zone of the reorganized

    chamber; or (3) resorption of phenocrysts in such

    magma (previously deeper and water-undersaturated)

    drawn to the top of the partially evacuated chamber

    and subsequently saturated with water, owing to

    bubble ascent and concentration near the roof of

    aqueous gas exsolved from still-deeper (untapped)

    parts of the reservoir during the climactic depressur-

    ization; or (4) similar resorption caused by CO2exsolution (thereby raising H2O activity) during as-

    cent of gas-saturated but formerly CO2-richer rhyolite

    magma from deeper in the reservoir; or (5) concen-

    tration at the top of the chamber (in response to such

    depressurization and reorganization) of interstitial

    melt expelled from a great reservoir of crystal mush

    that had underlain the zoned Bishop Tuff magma that

    erupted. The mush model is discussed in Section 7,

    below. Similarities in composition (Fig. 4) and in

    temperature(Bailey, 1978; Hildreth, 1979; Heumann,

    1999) between ER and late Bishop Tuff suggest that

    mixing with hotter deeper magma was limited, whilethe relatively elevated Ba content of ER (Fig. 4)

    suggests contributions either from dacitic magma or

    from resorption of sanidine-rich cumulates. Basaltic

    enclaves (49% SiO2) that reflect mafic recharge have

    been found in only one lava (680 ka) among the many

    ER-eruptive units (Bailey, 2004).

    4.3. In what sense was the structural uplift

    resurgent?

    Intracaldera resurgence was defined bySmith andBailey (1968) as structural uplift of the caldera floor

    by renewed buoyancy or intrusion of the viscous

    magma remaining in the postcollapse reservoir; but

    the term has sometimes been inappropriately conflated

    with postcalderaeruptiveactivity that may or may not

    accompany such uplift. Bailey et al. (1976) showed

    that structural uplift at Long Valley was largely

    contemporaneous with the 100-kyr interval of ER

    eruptions and was probably largely over by f 500

    ka. Some ER vents lie along or close to faults

    associated with the uplift, but the relative timing of

    individual eruptive units and the offset on long-active

    faults is seldom clear. The roughly circular area of

    uplift (Fig. 2) is f 10 km across and dips radiallyoutward at 1025j(Bailey, 1989). Lookout Mountain

    (677692ka), an ER cone in the NW moat, is outside

    the uplift (Figs. 2, 3), as are thick sections of ER

    concealed beneath other sectors of the moat.

    Thehigh point of the uplift is Gilbert Dome (2626

    m asl; Fig. 3), and if ER thickness is similar to that

    (622 m) in the Long Valley Exploratory Well (LVEW)

    f 2 km south, then the top of the subjacent Bishop

    Tuff would be f 2000 m asl, probably its maximum

    intracaldera elevation. This is 261 m higher than the

    top of the Bishop Tuff in the LVEW (at a site down-

    faulted within the medial graben; Fig. 3), 4 6 9 m

    higher than in well 44 16 in the west moat, and

    575 m higher than in well 6629 in the SE moat

    (Suemnicht and Varga, 1988; Bailey, 1989; McCon-

    nell et al., 1995). It seems likely that the fluidized

    primarysurfaceof the Bishop Tuff that ponded inside

    the caldera was virtually horizontal at the close of its

    eruption. Therefore, even though part of the excess

    elevation of the resurgent dome owes to the construc-

    tional pile of proximal ER, and part to differential

    compaction of the Bishop Tuff (which is much thicker

    in the low eastern third of the caldera; Hill, 1976;Bailey, 1989), doming of the top surface of the Bishop

    Tuff clearly demonstrates central uplift of at least 400

    m. Most of the uplift appears to have been during ER

    time, but what fraction may have continued episodi-

    cally is not clear. The 400-m total uplift in roughly

    100 kyr can be compared with f 1 m of renewed

    uplift in the last 25 years (Savage and Clark, 1980;

    Langbein, 2003), 10 times greater than the earlier rate.

    Drillcore from the LVEW (virtually central to the

    uplift) revealed in the 1.2-km-thick Bishop Tuff some

    10 phenocryst-poor intrusions, apparently sill-like andnot present in wells drilled peripheral to the uplift

    (McConnell et al., 1995). Compositionally, the sills

    are Ba-rich rhyolite much like the ER, and with a

    cumulative thickness off 330 m, they could account

    for most of the resurgent uplift. For a 10-km-wide

    domical uplift of 400 m, the apparent volume of

    inflation is about 10 km3, merely 10% of the volume

    of ER erupted. The conventional model that a resur-

    gent residual magma chamber buoyantly upwarps the

    cauldron block by reinflation or upward stoping is,

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    therefore, for Long Valley, no more compelling than a

    model of central uplift by injection of shallow sills or

    laccoliths into the thick intracaldera fill(McConnell et

    al., 1995).The fault system on the resurgent dome is domi-

    nated by NNW trends essentially parallel to those of

    rangefront faults north and south of the caldera (Figs.

    2, 3), butalsoparallel to the strike of steeply dipping

    structures and bedding in the metamorphic basement

    rocks (Rinehart and Ross, 1964). Radial and dome-

    concentric faults are inconspicuous. Thus, the struc-

    ture of the uplift appears to have been influenced more

    by (1) regional precaldera structures and (2) suscep-

    tibility of the shallow, subhorizontally layered Bishop

    Tuff to sill injection rather than by chamber-wide

    buoyancy. Location of the uplift nonetheless surely

    reflects the main locus of the reorganized postcaldera

    magma reservoir, which so voluminously supplied the

    ER. For the last half-million years, however, despite

    paths provided by the complex fault system(Fig. 3),

    there have been no further eruptions on the resurgent

    dome.

    4.4. North-central rhyolite chain

    The earliest of three clusters of post-resurgence

    rhyolites thatBailey (1989) termed Moat Rhyolite isa NW-trending chain of five units (orange in Fig. 3)

    crossing the NE sector of the resurgent dome, therefore

    not really in the caldera moat at all nor aligned along

    the ring-fault zone. In contrast to the voluminous ER,

    all are phenocryst-rich and of small eruptive volume,

    totaling f 1 km3. About 100 jC lower in FeTi-oxide

    temperature than the nearly aphyric ER, the north-

    central rhyolites are rich in quartz, plagioclase, sani-

    dine, hornblende, and biotite. SiO2contents (7475%)

    are similar to ER, but K2O (4.7%) and Ba (680715

    ppm) contents are significantly lower than ER(Fig. 4),probably as a result of sanidine fractionation.

    The four extrusive units yielded sanidine K Ar

    ages of 527F 12, 523F 11, 505F 15, and 481F10

    ka(Mankinen et al., 1986),thus potentially spanning

    an eruptive interval 46F 22 kyr long. The fifth and

    SE-most member of the chain(Fig. 3)is a granophyric

    intrusion in well CP-1 (Suemnicht and Varga, 1988),

    similar to the lavas in composition (74.2% SiO2) and

    mineralogy. Mafic enclaves (53.5% SiO2; Bailey,

    2004) occur in lava and agglutinate of the NW-most

    vent of the chain, but none have been found in any

    younger Long Valley rhyolite.

    4.5. Southeastern rhyolite cluster

    After an apparent hiatus off 120 kyr, another set

    of rhyolites erupted over an interval as long as f 75

    kyr, from a cluster of five vents (green inFig. 3) in the

    calderas low SE moat. Two of these vents arguably

    extend the trend of the north-central chain just dis-

    cussed, and two clearly lie along the ring-fault zone

    (Fig. 3), the others inboard. The extensive (12 km2)

    Hot Creek flow and the two small eastern lavas are

    quartz-free and crystal-poor (13% feldspars, biotite,

    cpx, FeTi oxides), whereas the central pair (striped

    green in Fig. 3) of the cluster are phenocryst-rich

    hornblende-biotite rhyolites like the north-central

    chain. All five, however, have f 76% SiO2 and

    500700 ppm Ba (Fig. 4). Altogether, the five add

    up to only f 1.5 km3, the Hot Creek flow being most

    of it. All have been dated (Mankinen et al., 1986;

    Heumann, 1999): sanidine yields 362F 8 ka for the

    northernmost lava and 333F 10 ka for the south-

    central lava, both crystal-rich. For the three pheno-

    cryst-poor units, sanidine gave 329 F 23 ka for the NE

    lava and 329F 3 ka for the SE lava, and for the Hot

    Creek flow obsidian gave 288F 31 ka (possibly tooyoung owing to Ar loss from glass?). Whatever

    process promoted reversion to crystal-poor rhyolite

    at about 330 ka, it was unique in the post-ER evolution

    of the Long Valley magma reservoir, because all other

    Long Valley rhyolites (527 to 100 ka) are rich in

    phenocrysts. Thermal rejuvenation by basalt injection

    is an unlikely explanation for these low-temperature

    rhyolites because the crystal-poor units are marked by

    small euhedral phenocrysts and lack xenocrysts or

    partly resorbed relicts of an earlier generation. A more

    likely process, high-silica melt extraction from crystal-rich felsic mush is discussed in Section 7.

    4.6. West moat rhyolites

    After another hiatus of about 150 kyr, a third

    cluster of moat rhyolites (blue inFig. 3)erupted west

    of the resurgent domefour small lava domes and the

    extensive West Moat Coulee (8.5 km2; as thick as 574

    m;Benoit, 1984). The coulee represents f 4 km3 of

    rhyolite lava but the four domes add up to only f 1

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    km3 more. Four of the rhyolite vents are along the

    ring-fault zone, while Deer Mountain lies f 2.5 km

    outboard of it (Fig. 3). All five have been dated

    (Mankinen et al., 1986; Heumann, 1999; Ring,2000). Oldest is the West Moat Coulee at 161 F 2

    ka, while the Dry Creek dome, the two Mammoth

    Knolls, and Deer Mountain yield overlapping ages in

    the range 11597 ka. All are phenocryst-rich (20

    30% quartz + sanidine + plagioclase + biotite + horn-

    blende + FeTi oxides), low-temperature rhyolites, but

    chemically they are of two kinds (Fig. 4): Deer

    Mountain and the coulee have high Ba (700 860

    ppm) and only 72 73% SiO2, whereas Dry Creek

    dome and the Mammoth Knolls are more evolved,

    with 7677% SiO2 and lower Ba (110200 ppm).

    4.7. The postcaldera Long Valley magma chamber

    Although Glass Mountain rhyolites totaled f 100

    km3, Bishop Tuff rhyolite f 600 km3, and Early

    Rhyolites f 100 km3, the 15 eruptive units of post-

    650-ka Long Valley rhyolite add up to only 7 or

    8 km3less thanthat released at Novarupta (Alaska)

    in 1 day in 1912 (Fierstein and Hildreth, 1992). The

    scarcity of tuff accompanying the three sets of moat

    rhyolite lavas suggests that any lost fallout volume is

    small. Despite the near-verticalstructural grain of thestratified metamorphic rocks (Rinehart and Ross,

    1964) that compose much of the foundered cauldron

    block, and despite the complex system of faults trans-

    ecting the resurgent dome(Fig. 3),there has not been

    a single eruptive leak on the uplift itself in the last

    half-million years.

    Additional evidence suggesting that the Long Val-

    ley magma chamber may have largely crystallized

    includes:

    (1) Volumetric eruption rate of postcaldera rhyolite

    wasf

    1 km

    3

    /kyr in ER time but has beenf

    0.01km3/kyr since 650 ka, a hundredfold decline.

    (2) Most of the 15 moat rhyolites (and all those

    younger than f 300 ka) were crystal-rich, low-tem-

    perature magmas, suggesting that active separation of

    melt from crystal mush has ceased.

    (3) Although teleseismic arrival-time tomography

    (Dawson et al., 1990; Wieland et al., 1995)appears to

    have identified diffuse low-velocity anomalies in the

    mid-crust, high-resolution tomography based on local

    earthquakes (Kissling, 1988; Romero et al., 1993)

    found no distinct low-velocity bodies in the upper

    crust beneath Long Valley caldera.

    (4) Present-day geothermal fluids beneath the south

    and southeast moat are supplied by eastward under-flow from western areas of younger magmatism

    outside the structural caldera, not from beneath the

    immediately adjacent resurgent dome (Sorey et al.,

    1991; Romero et al., 1993; Pribnow et al., 2003).

    (5) The 3-km-deep LVEW, virtually centered on

    the resurgent dome, is isothermal at 100 jC over its

    bottom 1000 m, requiring an astonishingly steep

    thermal gradient if there were residual 700 jC rhyo-

    litic magma in the upper crust beneath it.

    (6) Although self-sealing might isolate hydrother-

    mal convection cells promoting cooling at still deeper

    levels,Sorey et al. (1991)pointed out that deep wells

    elsewhere on the resurgent dome have kilometer-scale

    segments with near-linear thermal gradients near 40

    jC/km, suggesting only modest conductive heat

    flowinconsistent with survival of a subjacent up-

    per-crustal magma chamber.

    (7) Fluid-inclusion and oxygen-isotope studies of

    hydrothermally altered material from deep in LVEW

    (McConnell et al., 1997; Fischer et al., 2003) identi-

    fied a high-temperature (300350 jC) paleo-hydro-

    thermal system that appears to have died out soon

    after 300 ka (Sorey et al., 1991)perhaps not coin-cidentally the age of the last crystal-poor intracaldera

    rhyolites.

    (8) If basaltic resupply to the roots of the subcal-

    dera rhyolitic reservoir (Lachenbruch et al., 1976) had

    prolonged rhyolite crystallization to the present, it

    would seem anomalous that such postcaldera mafic

    magma has erupted nowhere immediately north or

    south of the structural caldera. Postcaldera eruptions

    of mafic and intermediate magma (most or all younger

    than 200 ka) are limited to a NS belt west of the

    structural caldera(Figs. 2, 5)where they are likely tohave influenced the thermal state of the Long Valley

    rhyolite reservoir only marginally.

    In summary, the compelling inference is that the

    formerly vigorous Long Valley magma chamber is

    moribund. If the recent (19792003) 80-cm uplift of

    the resurgent dome(Hill et al., 2002, 2003),attributed

    to an inflation source at a depth of 67 km(Langbein,

    2003), was caused by intrusion of a mafic dike, this

    would provide further evidence that the subcaldera

    rhyolitic reservoir, now penetrable, has crystallized.

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    5. Western postcaldera magmatism

    Because drilling(Suemnicht and Varga, 1988) has

    shown the ring-fault zone to lie as far as 5 km insidethe western wall of the topographic depression(Figs.

    2, 3, 5), all of the following eruptive groups vented

    outside the structural caldera: (1) the Mammoth

    Mountain dome complex; (2) >35 mafic scoria cones

    and lavas; (3) three crystal-poor dacite lavas periph-

    eral to Mammoth Mountain; and (4) a chain of four

    hybrid dacite lavasthat crosses the northwest wall of

    the caldera(Fig. 5). Products of the 60-odd vents are

    magmatically unrelated to the residual Long Valley

    reservoir (Fig. 4), and most or all are younger than

    about 200 ka. Of the many units erupted west of the

    ring-fault zone, only Deer Mountain (101F 8 ka) and

    the coarsely porphyritic rhyolite that mingled syner-

    uptively with the 650-year-old Deadman Creek and

    Glass Creek (Inyo) domes (Sampson and Cameron,

    1987) appear to represent residual or rejuvenated

    Long Valley magma.

    5.1. Mammoth Mountain dome complex

    Mammoth Mountain is a silicic dome cluster at the

    focus of a peripheral array of roughly contemporane-

    ous mafic vents(Fig. 5),in the same sense as Adams,Hood, Mazama, Newberry, Medicine Lake, Shasta, or

    the Lassen domefield in the Cascades or the San

    Francisco Peaks in Arizona. The eruptive volume of

    Mammoth Mountain is relatively small (4F 1 km3),

    though with 750 m of relief the edifice is imposing

    because draped over the high basement rim of the

    Long Valley depression. Although only f 13 vents

    are exposed (Fig. 5), the edifice consists of at least

    2530 overlapping domes and flows of trachydacite

    and alkalic rhyodacite (6571% SiO2)(Bailey, 1989,

    2004). They define a compositional continuum (Fig.

    4), but products with < 70% SiO2 are phenocryst-

    rich (hornblende + biotite + plagioclase + FeTi oxi-

    desFpyroxeneFNa-sanidine) and those with z

    70% SiO2 are generally crystal-poor (with the samesuite but generally including Na-sanidine and

    quartz). The Mammoth Mountain compositional

    array (Fig. 4) is distinct from those of Long Valley

    a nd t he M on o C ra te rs c ha in (Kelleher and

    Cameron, 1990; Ring, 2000; Bailey, 2004).

    Radiometric ages determined for Mammoth Moun-

    tain include eight units K Ar dated in the 1970s

    (Mankinen et al., 1986) and nine units dated by40Ar/39Ar incremental heating (Ring, 2000). Many

    of the KAr ages were for biotite separates shown

    by Ring (2000) to contain excess Ar, thus giving

    systematically older ages than coexisting feldspar. The

    commonly cited 25050 ka range of eruptive activity

    for Mammoth Mountain is therefore too long. Reli-

    ably precise ages for lavas (and a pumice fall) from

    most sectors of the edifice, and from top to toe, range

    from 111F 2 to 57F 2 ka. The Earthquake Dome (2

    km NE of Mammoth Mountain; Fig. 5) is of similar

    age (86F 2 ka) and composition (crystal-rich trachy-

    dacite; 66.4% SiO2), thus magmatically related to the

    main edifice as a flank dome. Magmatic eruptive units

    older than 111 ka might well be buried within the

    edifice, but there are none younger than 57 F 2 ka.The 40Ar/39Ar ages suggest that more than half the

    bulk of Mammoth Mountain erupted in the interval

    6757 ka(Ring, 2000).

    Not only is Mammoth Mountain far outside the

    Long Valley ring-fault zone, neither is it magmatically

    related to the Mono-Inyo chain, as sometimes

    asserted. (1) Mammoth Mountain is wholly older than

    the Mono-Inyo chain, the southern 13 km of which

    (Fig. 5) propagated episodically toward Long Valley

    only during the Holocene(Bursik and Sieh, 1989).(2)

    The trachydacites and alkalic rhyodacites of Mam-

    Fig. 5. Mammoth Mountain and its mafic periphery. Topographic margin of caldera basin and ring-fault zone (RFZ) as in Figs. 2 and 3.Vent

    symbols identified in inset. Additional silicic vents are concealed within the Mammoth Mountain edifice. Nearly all vents in the array depicted

    are monogenetic and erupted after 200 ka, but farther east there are no vents younger than f 300 ka, neither inside nor outside the caldera. The

    400-ft contours show that 11,053-ft Mammoth Mountain is a modest edifice (4F 1 km3) built atop a high basement ridge. Placename

    abbreviations as inFig. 3; in addition, CC = Crystal Crag; DP = Devils Postpile; HL = Horseshoe Lake; MP= Mammoth Pass; MR = Mammoth

    Rock; MS = Minaret Summit; ND = North Deadman Dome; PB = Pumice Butte; RC = Red Cones; RM = Reds Meadow. Three largest domes of

    rhyolitic Inyo chain are Deadman Creek (DC), Glass Creek (GC), and Obsidian Dome (OD); two slightly older mini-domes adjacent to GC are

    Cratered Dome (CD) and a southerly one unnamed. Vent alignments marked by dashed lines are NW wall hybrid dacites, mafic units along Fern

    Lake fault zone (FLFZ), and Red Cones. Drillholes mentioned in text include Long Valley Exploratory Well (LVEW) and Shady Rest (SR); four

    others are named as labelled on map.

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    layer of cinders midway through the pile suggests

    proximity to a buried vent.

    A third well 3 km farther SE (Figs. 3, 5; PLV-1;

    Benoit, 1984) encountered no mafic lavas at all in

    penetrating 687 m of 161-ka Moat Rhyolite lava and

    tuff that rests directly on ER, indicating that the mafic

    eruptions in (at least that part of) the west moat took

    place afterf 160 ka. This inference is supported by

    data for a fourth well, PLV-2(4 km N ofPLV-1;Figs.

    3, 5;Benoit, 1984), where 169 m of mafic lavas (f 8

    flows with soils and ash intercalated) overlie an 86-m

    package of Moat Rhyolite lava and tuff (not exposed

    at the surface), which again rests directly upon ER.

    Finally, and remarkably, a fifth well (Shady Rest;Figs.

    3, 5; Wollenberg et al., 1987) f 1.5 km east of

    Mammoth Knolls, at the foot of the resurgent dome,

    penetrated till, Moat Rhyolite, and Early Rhyolite,

    finding no mafic lavas at all. Farther east, none of the

    Fig. 6. Outline map of six successive magmatic foci in the Long Valley region. #1 encloses area of precaldera dacite (PCD) vents (3.5 2.5 Ma).

    #2 encloses area of >60 Glass Mountain (GM) vents for high-silica rhyolite (2.20.79 Ma). #3 is bounded by ring-fault zone of Long Valley

    caldera (LVC), which collapsed on eruption of the Bishop Tuff (0.76 Ma). #4 encloses the trachydacite-rhyodacite Mammoth Mounta in (MM)

    center (110 57 ka) and its peripheral array off 35 mafic vents (1608 ka). #5 encloses area above teleseismically anomalous domain(Achauer

    et al., 1986)in mid-crust beneath central core of (f 500.65 ka) Mono Craters (MC); arrows depict late Holocene propagation of dike-fed chains

    of rhyolite domes north and south of the core. #6 is the youngest focus (14 to 0.25 ka) at Mono Lake (not dealt with in detail in this paper),

    including vents at Black Point and both islands (Lajoie, 1968; Stine, 1987; Bailey, 1989; Kelleher and Cameron, 1990).Faults as in Fig. 2.

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    many wells on the resurgent dome (or south and east

    of it) have encountered mafic lavas. Vents for such

    lavas are limited to the west moat and areas still

    farther west and southwest(Fig. 5).Volumes of mafic lavas erupted are hard to recon-

    struct owing to burial in the west moat and to glacial

    erosion elsewhere, but most units are small. The most

    voluminous mafic units appear to be the andesites of

    Mammoth Pass and Devils Postpile and the pair of

    lava aprons just west of Lookout Mountain (Bailey,

    1989), all four of which had volumes in the range

    0.51 km3 (assuming average thicknesses in the

    range 50100 m). On the floor of the San Joaquin

    canyon, the severely glaciated basalt of The But-

    tresses, now a 1.5-km2 remnant as thick as 120 m,

    might once have been three times as big, thus likewise

    as voluminous as 0.5 km3. The Pumice Butte vent

    cluster south of Mammoth Mountain adds an addi-

    tional f 0.2 km3. As f 45 km2 of the west moat

    appears to be underlain by mafic lavas, where drilling

    suggests an average thickness of 200F 50 m, their

    total volume there might be roughly 9 km3. If the

    thickness of the mafic lavas (f 16 km2) that flowed

    down the south moat averages f 50 m, they add < 1

    km3 to the total mafic volume. In summary, then,

    although not well constrained, the total volume of

    mafic magma erupted from the 35-vent array sur-rounding Mammoth Mountain is probably >10 km3

    but is unlikely to exceed 15 km3.

    Ages of eruption of the many postcaldera mafic

    units remain inadequately known and are the object

    of ongoing work. The only patently postglacial unit

    among them is the basalt of Red Cones, f 8.5 ka

    (M. Bursik, unpubl. data). KAr ages for nine units

    (plus several duplicates) were published by Manki-

    nen et al. (1986), and 40Ar/39Ar ages for nine more

    were determined byRing (2000).Sixteen of the ages

    fall between 160F

    2 and 65F

    2 ka. The nominallyoldest determination is a whole-rock K Ar age of

    228F 82 ka for an andesite vent f 500 m SE of

    Mammoth Knolls (Fig. 5), but this low-precision

    result needs to be verified. The youngest is 31F 2

    ka for the basaltic apron south of Crestview near the

    calderas NW wall. The 9-km-long basalt tongue in

    the north moat gave a KAr age of 108 F 12 ka, and

    the stack of 3 south-moat lava flows near Casa

    Diablo yield 40Ar/39Ar ages in the range 160 98

    ka(Ring, 2000), apparently surmounting the contam-

    ination problems that had plagued previous attempts

    to date them by KAr(Mankinen et al., 1986). Four

    mafic lavas from the Inyo-4 drillhole were dated by40

    Ar/39

    Ar incremental heating (Vogel et al., 1994).Two near the top of the 319-m stack of 26 flows

    gave reasonable plateau ages of 161F14 and

    151F17 ka, consistent with the likelihood that the

    stack banks against the nearby West Moat rhyolite

    coulee (161F 2 ka; Ring, 2000), beneath which

    drillhole PLV-1 showed mafic lavas not to be present.

    The two samples near the bottom of Inyo-4, however,

    gave low yields of radiogenic Ar and highly dis-

    turbed spectra (owing to excess Ar or recoil or both)

    that were interpreted to yield a combined age

    (415F 53 ka) that, pending verification, should not

    be accepted.

    Whether all 35 mafic eruptive units are younger

    than 160 ka remains to be determined but seems

    possible. Some have considered the undated basalt of

    The Buttresses in the San Joaquin canyon to be

    much older (e.g., Cousens, 1996), but Bailey

    (2004) pointed out that its dike-fed vent complex

    is on the present-day canyon floor, andBailey (1989)

    showed that it directly underlies the dacite of Rain-

    bow Falls, which is now well dated at 97F 1 ka

    (Ring, 2000).

    The youngest mafic products actually erupted inthe Long Valley area are andesitic enclaves in the 650-

    year-old Inyo Domes, found only in the coarsely

    porphyritic mixing member present in the Glass Creek

    and Deadman Creek domes (Varga et al., 1990). It

    may be, however, that dike ascent such as fed the

    mafic vent array for the last 160 ka is likewise

    responsible (though as yet unerupted) for (1) ongoing

    upper-crustal seismicity and CO2 discharge beneath

    Mammoth Mountain(Hill, 1996);(2) numerous long-

    period volcanic earthquakes at focal depths of 10 25

    km in a cluster that extends 10 km WSW frombeneath Mammoth Mountain to the Devils Postpile

    area (Pitt et al., 2002), spatially coinciding with the

    vent array in that sector; and (3) the ESE-striking

    array of late Holocene phreatic craters at the north toe

    of Mammoth Mountain(Bailey, 1989).

    Compositionally, the peripheral mafic array ranges

    continuously from trachybasalt to trachyandesite (47

    to 58.5% SiO2), plus 3 dacites to be discussed in

    Section 5.3. Nearly all are mildly to transitionally

    alkalic, except the Holocene basalt of Red Cones,

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    which is subalkalic (Vogel et al., 1994; Cousens,

    1996; Bailey, 2004). The general alkalinity of the

    mafic magmatic rocks is consistent with such material

    having provided a parental contribution to the con-temporaneous trachydacite to alkali-rhyodacite suite

    of Mammoth Mountain. In contrast, silicic rocks of

    the generally older Long Valley suite (Glass Mountain

    through Moat Rhyolites) and the younger Mono

    Craters suite are subalkalic(Fig. 4).

    The only fairly primitive eruptive units in the mafic

    array are the basalts of The Buttresses and of Horse-

    shoe Lake, each in the range 47 49% SiO2 with

    f 10% MgO and 160210 ppm Ni, but these are

    very enriched in Ba, Sr, and LREE, consistent with

    their alkalinity(Cousens, 1996).The subalkalic basalt

    of Red Cones, with 50% SiO2, 8% MgO, and 120

    ppm Ni, is the only other relatively primitive Quater-

    nary basalt so far recognizedin the array. The 30-odd

    additional samples analyzed (Cousens, 1996; Bailey,

    2004), which representf 20 separate eruptive units,

    contain only 2.5 7% MgO and < 100 ppm Ni, as do

    lava flows in the Inyo-4 drillhole(Vogel et al., 1994).

    Like many intracontinental mafic lavas, these have

    high 87Sr/86Sr (0.70520.7067) and low 143Nd/144Nd

    (0.5124 0.5128) (n =35; Cousens, 1996). There is

    extensive xenocrystic and chemical evidence for

    crustal assimilation by many of the mafic units(Man-kinen et al., 1986; Vogel et al., 1994; Cousens, 1996;

    Ring, 2000), but even the more primitive basalts

    appear also to contain a contribution from enriched

    mantle lithosphere (Nielsen et al., 1991; Cousens,

    1996). The relative contributions of partial melts of

    mafic to silicic crustal rocks and of enriched upper

    mantle needs clarification.

    5.3. Crystal-poor dacites peripheral to Mammoth

    Mountain

    Three widely separated eruptive units of pheno-

    cryst-poor dacite lava lie near the foot of Mammoth

    Mountain (Fig. 5). (1) The dacite of Rainbow Falls

    (67% SiO2) is a 6-km-long glaciated coulee on the

    floor of the San Joaquin canyon that erupted f 2 km

    SW of the toe of Mammoth Mountain. (2) The dacite

    of upper Dry Creek (67.8% SiO2), also glaciated and

    partly concealed by basalt and surficial deposits,

    crops out from 1 to 3 km north of the base of

    Mammoth Mountain. Both have f 5% phenocrysts

    of plagioclase>opxf cpx>FeTi oxides. They yield

    ages of 97F 1 and 103F 9 ka, respectively (Ring,

    2000; Mankinen et al., 1986). (3) The undated dacite

    of McCloud Lake crops out f 1 km south of thebase of Mammoth Mountain as glaciated lava rem-

    nants resting on granitic basement along the up-

    thrown side of a N-striking fault (Bailey, 1989).

    With only 1 2% plagioclase>hornblendeF sparse

    cpx, it is even crystal-poorer than the other two.

    Their relatively alkalic compositions suggest that the

    three crystal-poor dacites are related to the adjacent

    Mammoth Mountain system, perhaps as interstitial

    melts that separated from trachyandesitic crystal

    mush. In contrast to the next set of dacites discussed,

    they lack obvious xenocrysts or detectable evidence

    for mixed parentage.

    5.4. Northwest wall hybrid dacite chain

    Crossing the NW wall of the topographic caldera

    basin is a NW-aligned chain (Fig. 5) of four crystal-

    rich silicic lavas (61 66% SiO2) called olivine-

    bearing quartz latite by Rinehart and Ross (1964),

    quartz latite by Bailey (1989), and hybrid

    dacites by Bailey (2004). The chain includes two

    small domes (each < 0.005 km3) and twomodest lava

    flows (each f 0.04 km3

    ). Ring (2000) and Bailey(2004) provide petrographic evidence for complex

    magma mixing and phenocryst disequilibrium, in-

    volving (1) trachydacite similar to that of Mammoth

    Mountain, (2) rhyolite containing quartz and K-rich

    sanidine similar to Long Valley rhyolites, and (3)

    mafic enclaves and derivative xenocrysts of olivine,

    cpx, and calcic plagioclase. 40Ar/39Ar ages deter-

    mined by Ring (2000) are 40F 1 and 39F 1 ka for

    the NW pair and 30F 1 and 27F 1 ka for the SE pair

    of lavas comprising the chain, all four ages being for

    K-rich sanidine. Sorey et al. (1991) reported that thepresent interval of hot-spring discharge in Long Val-

    leys south moat began f 40 ka and is thought to be

    supplied by underflow in shallow aquifers from an

    unidentified deeper heat source in the west moat. The

    timing may be a coincidence but, if the 40-ka start-up

    time is accurate, intrusions associated with the hybrid

    dacite chain are more plausible a heat source than

    Mammoth Mountain (dormant since 57 ka) or the

    650-year-old Inyo dike (only 7-m thick; Eichelberger

    et al., 1985).

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    5.5. Vent alignments

    Much attention has been paid the 8-km-long NS

    alignment of Holocene Inyo rhyolite domes andcraters (Miller, 1985; Section 6 below). Other vent

    alignments (Figs. 2, 5) include: (1) the NW-wall

    chain of hybrid dacites just discussed, which strikes

    N45jW; (2) the principal vent array of Mammoth

    Mountain, which strikes N60jW; (3) the array of

    late Holocene phreatic craters that strikes N70jW

    across the north toe of Mammoth Mountain (Bailey,

    1989); (4) a chain of five phenocryst-poor mafic

    vents that strikes N45jW from the west moat along

    the Fern Lake fault zone (Fig. 5; Bailey, 1989); (5)

    clusters of phreatic craters aligned roughly NW

    along a fault zone just west of Deer Mountain

    (Mastin, 1991); (6) the chain of 500-ka rhyolites

    that strikes N45jW across the northeast slope of the

    resurgent dome (Figs. 2, 3); and (7) fault-influenced

    alignments of ER vents that trend N2040jW across

    the resurgent dome (Fig. 3). Predominance of north-

    westerly alignments is probably related to the NNW

    trend of the rangefront fault system and to the

    roughly parallel strike of near-vertical bedding and

    structures in the metamorphic basement (Rinehart

    and Ross, 1964).

    Many vents for the southeast- and west-moatrhyolite groups (Figs. 2, 3) appear to be arranged,

    however, along or adjacent to the buried ring-fault

    zone, as likewise are early postcaldera Dome 7403

    and ER Lookout Mountain. As Deer Mountain dome,

    however, which is the only moat rhyolite clearly

    outsidethe ring-fault zone, lies 3 5 km NW of coeval

    100-ka moat rhyolites, its intrusive feeder may also

    have been influenced by the NW-trending basement

    structures. On the other hand, a line connecting the

    Red Cones vent pair (the only Holocene basaltic

    eruptive unit) strikes N25j

    E (Fig. 5), presumablythe orientation of a mutual feeder dike. This is roughly

    parallel to the NNE trend of a possible dike inferred to

    have been emplaced beneath nearby Mammoth

    Mountain during an extended earthquake swarm in

    1989(Hill et al., 1990).

    The NS alignment of the Inyo chain (N7jW for

    the three 650-year-old domes) is apparently unique.

    Its feeder dike may have been controlled, at least in

    the shallow crust, by the Hartley Springs fault system,

    which swings to a nearly southerly trend as it transects

    the caldera wall (Fig. 2; Bailey, 1989; Bursik et al.,

    2003).

    The major concentrations of magmatism in the

    Long Valley area, however, have been expressed bynon-linear, roughly equant domains marked by clus-

    ters of scattered eruptive vents (Fig. 6): (1) precaldera

    dacite and andesite vents concentrated just northwest

    of the later site of the caldera, but nowhere else in the

    region (Bailey, 1989). (2) the Glass Mountain con-

    centration of >60 non-aligned high-silica rhyolite

    vents 3 8 km outside the ring-fault zone; (3) the

    Bishop Tuff-Early Rhyolite-Moat Rhyolite sequence

    that issued from a reservoir ovoid in plan view

    beneath the central part of the caldera; and (4)

    trachydacitic Mammoth Mountain and its surrounding

    array of >40 mafic and dacitic vents. Relative to these

    major long-lived domains, each the surface expression

    of a large volume of mantle and deep-crustal partial

    melting, the local alignments are shallow second-

    order features. Only in the continuous linear array of

    >40 rhyolitic vents composing the young Mono-Inyo

    chain has shallow magma ascent been utterly domi-

    nated by upper-crustal tectonics.

    6. Mono-Inyo chain

    Extending 25 km north from the NW corner of

    Long Valley, the Mono-Inyo chain (Fig. 2) is a

    sickle-shaped single-file alignment of rhyolite vents,

    mostly of Holocene age. The Mono chain, forming

    the arcuate segment of the sickle, consists off 28

    domes and coulees, several associated explosion

    craters and ejecta rings, and an extensive apron of

    pumiceous fall, flow, and reworked deposits (Bailey,

    1989; Bursik and Sieh, 1989). As conventionally (but

    arbitrarily) designated, the Inyo chain refers to the

    rectilinear handle of the sickle, the segment repre-sented by an additional seven rhyolite domes (and

    several phreatic craters) that strikes south from where

    the arcuate segment impinges on the rangefront fault

    system (Fig. 2). Continuity of the chain of virtually

    contiguous Holocene rhyolite vents demands that the

    Mono-Inyo chain represent in some sense a coherent

    magmatic system. Farther north, in and adjacent to

    Mono Lake, however, a cluster of young basalt-

    dacite-rhyodacite vents (Fig. 6; not dealt with in this

    paper), is compositionally different (Lajoie, 1968;

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    Stine, 1987; Bailey, 1989; Kelleher and Cameron,

    1990) and is best regarded as a magmatic subsystem

    independent of the rhyolitic reservoir that feeds the

    Mono-Inyo chain.

    6.1. Mono Craters chain

    For the Mono chain, all lavas but one are high-

    silica rhyolite (75.477% SiO2). Major element (and

    most trace-element) contents are quite similar to

    those of Glass Mountain and the early Bishop Tuff

    (Fig. 4), the principal compositional feature distin-

    guishing the Mono domes being somewhat higher

    FeO* content (1.0 1.3 wt.%). Half of the Mono

    domes have 03% phenocrysts and the rest 3 8%

    (Wood, 1983; Kelleher and Cameron, 1990). The

    exception is an undated crystal-rich rhyodacite

    (68% SiO2), substantially older than any exposed

    Mono-Inyo rhyolites. All but four off 27 rhyolite

    lavas are of Holocene age; three are f 13 ka and one

    f 20 ka (Wood, 1983; Bursik and Sieh, 1989).

    Single-crystal 40Ar/39Ar ages for sanidine from pre-

    Holocene rhyolitic ash layers intercalated with lacus-

    trine silts of Mono Lake, however, suggest that as

    many as 15 explosive eruptions took place before 20

    ka, with a few as old as 5055 ka(Chen et al., 1996;

    Kent et al., 2002). This appears to require that one orseveral older explosive vents be concealed by the

    Mono domes currently exposed (Bursik and Sieh,

    1989).

    It was speculated that the arcuate trend of the Mono

    chain is controlled by a Mesozoic structure (Kistler,

    1966; Bailey, 1989), but the exposure is inadequate to

    verify the implausibility of the suggestion. More

    attractive is the proposal by Bursik and Sieh (1989)

    that the arcuate alignment represents the extensional

    margin of a pull-apart basin between NNW-trending

    oblique-slip faults having a dextral component.Straightening of the Holocene chain where the arcuate

    segment meets the rangefront fault zone (Fig. 2) is

    consistent with fault control of shallow dike propaga-

    tion farther southward; the east-dipping Hartley

    Springs fault zone, which remains active (Bursik et

    al., 2003), has dropped the Bishop Tuff f 135 m

    down to the east, thus yielding a 760-kyr average

    vertical displacement off 0.18 m/kyr.

    Estimates of the magma volume erupted from the

    Mono chain range from f 5 km3 (Wood, 1983)to 8.5

    km3 (Bursik and Sieh, 1989), the amount of lost and

    concealed pyroclastic deposits being the main uncer-

    tainties. Lava volume is f 4 km3, the largest units

    being the North and South Coulees at f 0.5 km3

    each. Wood (1983) pointed out a 4-fold increase in

    volumetric eruption rate atf 3 ka, an earlier Holo-

    cene rate off 0.2 km3/kyr jumping to f 0.8 km3/kyr

    for the last three millennia and coinciding with a

    switch from crystal-poor to virtually aphyric rhyolite.

    The four southernmost Mono domes are younger than

    5 ka, and South Coulee (Fig. 2) is part of the 1.3-ka

    South Mono eruptive episode (Bursik and Sieh,

    1989). The youngest Mono eruptions apparently is-

    sued from a 6-km-long dike that released thecomplex

    North Mono episode 660F 20 years ago (Sieh and

    Bursik, 1986), which included f 0.22 km3 of pyro-

    clastic fall and flow deposits and five separate lavas

    (0.44 km3), including North Coulee and Panum Cra-

    ter, all at the north end of the chain(Fig. 2).There has

    thus been a tendency for the Mono chain to propagate

    both northward and southward in the late Holocene

    (Fig. 6). This tendency continued with southward

    propagation (Mastin, 1991; Bursik et al., 2003) of

    the Inyo dike, serial eruptions of which (in the mid-

    14th century) followed the North Mono eruption by at

    most a few years (Miller, 1985; Sieh and Bursik,

    1986).

    6.2. Inyo chain

    The 10-km-long Inyo chain(Figs. 1, 4)consists of

    7 rhyolitic lava domes, several phreatic craters, and a

    modest composite apron of pyroclastic fall and flow

    deposits(Miller, 1985; Sampson and Cameron, 1987).

    The oldest unit is North Deadman dome (f 0.04 km3;

    75% SiO2), undated but probably mid-Holocene (46

    ka), followed by Wilson Butte (f 0.05 km3; 77%

    SiO2), which erupted about the same time as the 1.3-ka South Mono episode. Both domes are crystal-poor

    rhyolite. Wilson Butte is similar compositionally and

    petrographically to the Mono domes and would cer-

    tainly be considered a Mono dome were it not for the

    45j change in trend of the chain (Fig. 2). North

    Deadman dome is compositionally intermediate (Fig.

    4; Sampson and Cameron, 1987) between Wilson

    Butte and the crystal-poor lower-silica rhyolite that

    dominated the youngest Inyo eruptive episode 650

    years ago. Two crystal-poor mini-domes (each

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    f 0.001 km3) just north and south of the large Glass

    Creek dome(Fig. 5)have 7374% SiO2 and erupted

    after Wilson Butte but prior to the major 14th century

    Inyo eruption, the products of which they composi-tionally resemble(Sampson and Cameron, 1987).

    Injection of the Inyo dike (Eichelberger et al.,

    1985) in the mid-14th century led to sequential

    eruption of Deadman Creek, Obsidian, and Glass

    Creek domes(Figs. 2,5), each preceded by substantial

    pyroclastic outbursts (Miller, 1985), the last of which

    was followed by phreatic eruptions at nearby Inyo

    Craters (Mastin, 1991). Total volume erupted during

    this episode was estimated byMiller (1985)to be 0.4

    km3 of lava and 0.22 km3 of pyroclastic ejecta.

    Compositionally, the mid-14th century Inyo erup-

    tion was unusually complex (Fig. 4; Sampson and

    Cameron, 1987; Vogel et al., 1989). In addition to

    crystal-poor (2 3% crystals; finely porphyritic)

    zoned rhyolite (70 74% SiO2) that dominated the

    eruptive products, a very crystal-rich rhyodacite

    (71.3F 1% SiO2; 25 40% crystals; coarsely por-

    phyritic) piled up over the vents of the Deadman

    Creek and Glass Creek domes late in their extrusive

    episodes and mingled (to a limited extent) locally with

    the coerupted crystal-poor magma. Evidently having

    been stored separately, the crystal-rich magma was

    f 100 jC cooler and chemically unrelated to thecrystal-poor one, which has much higher K, Rb, Zr,

    Y, and REE (and lower Ti, Mg, Ca, and Sr) at

    equivalent SiO2 contents. In addition to the silicic

    magmas, andesitic enclaves (f 60% SiO2) are present

    in the crystal-rich central parts of both domes (Varga

    et al., 1990).

    The main crystal-poor magma was itself zoned

    (7074% SiO2), yielding smoothly linear composi-

    tional arrays (e.g., 1.32.6 FeO* and 2651420 ppm

    Ba), which are continuous but show an apparent

    tendency toward volumetric bimodalism (Sampsonand Cameron, 1987; Vogel et al., 1989). To explain

    the arrays, Sampson and Cameron (1987) suggested

    back-mixing between two slightly zoned silicic mag-

    mas that had earlier fractionated at higher pressure,

    while Vogel et al. (1989) called for mixing between

    dacitic and rhyolitic end-member magmas. Their

    high-silica endmember is similar to Mono domes

    rhyolite, and their dacitic end-member is much like

    the 40-ka hybrid dacite lavas on the caldera wall, right

    between the Glass Creek and Deadman Creek domes.

    Bailey et al. (1976)had suggested that the crystal-

    poor phase might be Mono domes magma (which is

    thus partly right) and that the crystal-rich phase is

    Long Valley magma (which appears to be whollyright). The compositional and petrographic similarity

    of the crystal-rich Inyo phase to t he nearby Moat

    Rhyolite of Deer Mountain (Fig. 4) was pointed out

    bySampson and Cameron (1987). Moreover,Reid et

    al. (1997) identified, in both the 100-ka Deer Moun-

    tain and the 0.65-ka crystal-rich Inyo phase, zircon

    populations with crystallization ages that cluster

    around 230 ka. Residual or thermally rejuvenated

    Long Valley magmatic mush is implicated.

    The significance here is that the 14th century Inyo

    eruption tapped a magma volume at the confluence

    of (1) the Long Valley residue, (2) the southward-

    advancing Mono domes high-silica rhyolite, (3) the

    western mafic array, and (4) through the hybrid

    dacite component, a contribution from Mammoth

    Mountain (as well as another one from Long Valley).

    It may notbe a coincidence, therefore, that seismic

    refraction profiles (twice, in 1973 and 1983) identi-

    fied reflections from a shallowly dipping low-veloc-

    ity horizon(lens?) at a depth off 7 km beneath the

    NW moat (Hill, 1976; Hill et al., 1985), virtually

    adjacent to this unique magmatic confluence. Be-

    cause the Inyo dike had advanced southward (Mas-tin, 1991; Bursik et al., 2003) from the northerly

    domain of its Mono rhyolite component, if the

    reflector does represent a magma lens, then it could

    be either the hybrid dacite reservoir or the crystal-

    rich Long Valley residue, or both. Equilibration

    pressure calculated for the crystal-rich (Long Val-

    ley-type) Inyo magma (Vogel et al., 1989), based on

    Al-in-hornblende geobarometry, is 2.3F 0.5 kb,

    equivalent to a depth of f 7F 1.5 km. For the

    crystal-poor Inyo magma, both this method (Vogel

    et al., 1989) and the water contents of melt inclu-sions trapped in phenocrysts (45 wt.% H2O) from

    pumiceous Inyo fallout (Hervig et al., 1989) suggest

    shallower storage (36 km), presumably north of the

    caldera for the Mono component at least. Nonethe-

    less, a dike is only a feeder, and it remains specu-

    lative to interpret from the eruptive sequence the

    preeruptive distribution of magma storage or the

    withdrawal dynamics, differential transport, and na-

    ture of confluence of magmas from discrete zones or

    elements of the reservoir(s).

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    7. Discussion

    7.1. Ring-fault zone and Long Valley caldera

    Because the ring-fault zone is so far inboard of the

    topographic wall(Figs. 2, 3, 5), Mammoth Mountain,

    much of the mafic array, and the Mono-Inyo chain all

    lie well outside the structural caldera, consistent with

    differences in composition, and therefore should not

    be considered magmati c successors of the Long

    Valley reservoir. Intersystem contiguity is recognized

    only in the west, where mafic magma may have

    reheated and remobilized the margin of the mushy

    granitic Long Valley residue, engendering the min-

    gling and mixing conspicuous in the NW moat.

    The ring-fault zone is not a single fault but a buried

    set of nested step-down faults, as supported by seis-

    mic refraction profiles (Hill et al., 1985), gravity

    modeling(Carle, 1988),and drillhole data(Suemnicht

    and Varga, 1988; Bailey, 1989). The outboard location

    of Dome 7403 at the calderas NE margin may reflect

    such a broad zone of step faults. The zone may not be

    everywhere smoothly elliptical as portrayed, especial-

    ly in the west, where subsidence could have utilized

    precaldera faults of the left-stepping rangefront sys-

    tem. Offsets along that inherited en-echelon fault

    system may have locally conveyed a jigsaw patternto the western structural margin, which might in turn

    have controlled (1) the outboard dike that fed moat

    rhyolite to 100-ka Deer Mountain; (2) the path of the

    Long Valley-type magma that later reached the NW

    moat to mix with the 4027 ka hybrid dacites and

    0.65 ka Inyo rhyolite; (3) offsets on the Discovery

    fault zone of Suemnicht and Varga (1988); and (4)

    ascent of the deep thermal water that flows eastward

    in shallow aquifers to the active geothermal areas in

    south-central Long Valley.

    7.2. Significance of several discrete magma systems

    Starting around 4.5 Ma, extensional unloading

    enhanced partial melting of the upper mantle beneath

    the Long Valley region, inducing coalescence and

    ascent of basaltic magmas. Distributed basaltic intru-

    sion progressively warmed the lower crust and fed

    many mafic eruptions scattered within a 10040-km

    belt that stretched from the High Sierra to the Adobe

    Hills (Fig. 1) but centered on the future site of Long

    Valley. The subsequent magmatic history is funda-

    mentally one of local concentrations, focussing of

    basaltic injection and consequent crustal partial melt-

    ing beneath particular domains within this broad belt(Fig. 6). The first focus was beneath a 20-km-wide

    zone centered on what is now the NW margin of the

    caldera, where numerous andesites and dacites erup-

    ted from San Joaquin Mountain to Bald Mountain

    (Bailey, 1989)between 3.5 and 2.5 Ma. This zone of

    distributed crustal magmas failed to coalesce, became

    apparently moribund after 2.5 Ma, and was marked

    by no further eruptions until after f 160 ka. The

    mantle-driven focus of crustal melting later shifted

    f 20 km east, to Glass Mountain where at least 60

    eruptions of high-silica rhyolite between 2.2 and 0.79

    Ma are the evidence for growth and eventual integra-

    tion of a major crustal pluton capable of sustained

    fractionation of high-silica, low-Sr melt (Mahood,

    1990; Metz and Mahood, 1991; Metz and Bailey,

    1993). Whereas no rhyolite at all had erupted from

    the earlier aborted andesite-dacite focus to the west

    (Fig. 6), the thick zone of partially molten crust that

    supplied Glass Mountain rhyolite eruptions for 1.4

    Myr intercepted all mantle-derived magma batches

    (required for its thermal sustenance), thus permitting

    no basalt, andesite, or dacite to reach the surface

    during its long interval of strictly high-silica rhyoliteeruptive activity.

    Around the time of the last eruption of Glass

    Mountain rhyolite (790 ka) but before the caldera-

    forming Bishop Tuff eruption (760 ka), the mantle-

    driven focus of crustal melting shifted or drifted

    westward f 20 km to yet a third area, abandoning

    its long-stable position beneath Glass Mountain and

    thermally energizing instead a zone that became

    central Long Valley, embracing the large Bishop Tuff

    magma reservoir and the subsequent locus of ER

    eruptions and resurgent uplift. Because there has beenno postcaldera magmatism in either the Glass Moun-

    tain domain or the eastern third of the caldera (except

    early Dome 7403), and because heat flow in both

    areas approximates only the Basin and Range average

    (Lachenbruch et al., 1976), the westward shift of

    magmatic focus was evidently complete and categor-

    ical. Just as during the Glass Mountain episode, no

    mafic or intermediate magma reached the surface

    through or peripheral to the silicic reservoir during

    the central Long Valley episode (790 300 ka), al-

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    though a minor dacite component in the Bishop Tuff

    (Hildreth and Wilson, in review) and mafic enclaves

    in two small postcaldera rhyolite units (Bailey, 2004)

    indicate its coexistence beneath the rhyolitic chamber.The complete absence of peripheral mafic magmatism

    during the extended Glass Mountain and main Long

    Valley intervals implies that intrusion of mantle-de-

    rived basalt remained tightly focussed beneath these

    successive domains of exceptionally voluminous rhy-

    olitic magma generation. Secular westerly drift of the

    mantle-derived focus of crustal intrusion helps explain

    the Glass Mountain paradoxthat allknown pre-

    caldera rhyolites were in the northeast, that the caldera

    subsided most deeply in the northeast, but that post-

    caldera eruptive and hydrothermal activity have been

    entirely farther west.

    The most recent shifts of mantle-driven magmatic

    focus(Fig. 6)have been principal elements discussed

    in this paper. The fourth focus started up f 160 ka,

    engendering the distributed (but compactly delimited)

    array off 35 mafic vents (Figs. 2, 5), additionally

    producing f 30 trachydacite rhyodacite eruptions

    from the Mammoth Mountain core of the array, and

    probably reenergizing the edge of the crystallizing

    Long Valley reservoir to yield the 160100 ka west

    moat rhyolites. The fifthmajor focus started up f 50

    ka, 25 30 km north of Mammoth Mountain, beneaththe central part of what became the Mono Craters

    chain. The new system progressively expanded north

    and south, its eruptive frequency increasing markedly

    in the mid-to-late Holocene. Because eruptive prod-

    ucts along the central (arcuate) part of the Mono chain

    are almost exclusively crystal-poor high-silica rhyo-

    lite, nearly identical to those of long-lived Glass

    Mountain, it seems reasonable to infer that a mushy

    pluton capable of supplying recurrent batches of

    highly evolved melt has likewise grown in the middle

    crust here (as suggested by teleseismic P-wave delays;Achauer et al., 1986). Just as during the active life-

    times of the Glass Mountain and Long Valley rhyolite

    systems, non-rhyolitic magma is now prevented by

    the Mono Craters silicic reservoir from erupting

    centrally. Mafic products are recognized peripherally,

    as late Pleistocene basalts at June Lake and Black

    Point(Figs. 2, 6),and as mafic enclaves within three

    of the 28 Mono domes (one Pleistocene rhyodacite

    and two early Holocene rhyolites; Bailey, 1989;

    Kelleher and Cameron, 1990).

    The evidence that crustal magma systems are

    energized by distributed intrusion (not underplat-

    ing) of mantle-derived basalt, which in turn is not

    uniformly distributed but is more intensely concen-trated in local domains, has been elaborated previous-

    ly(Hildreth, 1981; Hildreth and Moorbath, 1988). The

    model envisages that prolonged focussing at each

    domain promotes thermal and mechanical feedback

    between entrapment and crystallization of basalt,

    enhancement of lower-crustal ductility and melting,

    and maintenance of a buoyancy barrier. Such long-

    lived focussing is intense beneath large arc volcanoes

    and likewise beneath intracontinental centers like

    those inFig. 6. Salient points include the following:

    (1) Processes entail not just melting of older crustal

    rocks but partial remelting of young mafic intrusions

    and their differentiates, thermally induced by recurrent

    pulses of basaltic intrusion and crystallization.

    (2) The partial melting zone is not a magma

    chamber but rather, a plexus of dikes, pods, and

    mushy differentiated intrusions, where ductile defor-

    mation promotes extraction, aggregation, and blend-

    ing of varied melts.

    (3) The melt-fractions in such zones wax and wane

    in response to basaltic influx and to losses by ascent

    of aggregated hybrids.

    (4) Each focus has its own deep melting zone ofreduced density, usually impenetrable by primitive

    basalts, whereas, peripheral to such foci, more prim-

    itive batches (not intercepted and hybridized) can

    ascend to produce monogenetic cones.

    (5) Crustal thickness can be significant, by imparting

    to magmas the chemical signature of pressure-depen-

    dent residual phases (notably garnet) and by increasing

    intracrustal path length (increasing opportunities for

    hybridism), but age and composition of the varied

    crustal lithologies melting are likewise important.

    (6) Deep crustal melting zones feed upper-crustalmagma reservoirs (some by intermittently mobilizing

    diapirically to produce mushy differentiated plutons),

    and derivative mush columns consisting of cumulates

    and migmatized protoliths track the ascent paths that

    penetrate much of the crust.

    Extension alone is insufficient to promote such a

    major crustal magma system. Intensely focussed

    basaltic injection into the lower crust is the key.

    Contemporaneous with Long Valley magmatism,

    Quaternary extension has been great in nearby Fish

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    Lake, Eureka, Deep Springs, Saline, Panamint, and

    Death Valleys (Fig. 1), but Quaternary magmatism

    has been sparse there. Merely 3040 km southeast,

    Round Valley (Fig. 1) represents another left-step-ping offset in the Sierranrangefront extensional fault

    system (Bateman, 1992), similar in size and tectonic

    style to that at Long Valley, but it has remained

    virtually nonvolcanic.

    7.3. Late PleistoceneHolocene activity and current

    unrest

    The greater Mammoth Mountain and Mono-Inyo

    systems are not magmatic daughters of Long Valley

    but are, instead, new and mutual ly independent

    domains of crustal melting driven by newly activated

    foci of elevated melt production and ascent in the

    locally subjacent mantle. After caldera collapse, there

    were no mafic eruptions in or near Long Valley for

    500 kyr, and the array of 35 mafic vents erupted since

    f 160 ka isalmost wholly west of the ring-fault zone

    (Figs. 2, 5).

    The post-160-ka array of mafic vents (and the dikes

    that fed them) are viewed as part of the spatially

    focussed basaltic flux intrinsic to generating the

    110 57 ka Mammoth Mountain silicic anomaly at

    its center. Mammoth Mountain produced as many as30 silicic eruptive episodes during its f 50-kyr-long

    lifetime, many of the most voluminous units having

    been extruded around 67 ka(Ring, 2000),but for the

    lastf 57 kyr, there have been none. Although not all

    have yet been dated, the mafic vents close to Mam-

    moth Mountain (with one or two exceptions) appear to

    have erupted in the interval 16060 ka, thus starting

    earlier but largely overlapping the 11057 ka interval

    of silicic activity. Most of the trachydacite lavas that

    dominate Mammoth Mountain, moreover, contain

    mafic enclaves, demonstrating mafic-and-silicic mag-matic contemporaneity. Although both appear to have

    ceased erupting soon after 60 ka, a clear exception is

    Red Cones, a pair of early Holocene basaltic scoria

    cones (and derivative lava apron) just 4 km SW of the

    toe of Mammoth Mountain(Fig. 5),which might thus

    signify a recent mantle-magmatic revival.

    If the 1989 shallow seismic swarm directly beneath

    Mammoth Mountain did represent emplacement of a

    NNE-trending dike as modeled on the basis of earth-

    quake distribution(Hill et al., 1990) and deformation

    (Langbein et al., 1995), the dike orientation would be

    athwart previous local vent alignments except thatof

    the Red Cones pair, which is likewise NNE(Fig. 5). If

    the 1989 dike penetrated as shallow as the 13 kmdepth estimated, this would support the inference that

    the silicic reservoir had by now solidified (or, much

    less likely, were shallower still). Also supporting the

    notion of a local mafic-magmatic revival is the ongo-

    ing sequence (beneath and southwest of Mammoth

    Mountain) of long-period (LP) volcanic earthquakes

    at depths of 1025 km (Hill, 1996; Pitt et al., 2002).

    The LP sequence coincides areally with the mafic vent

    array in the Red Cones-to-Devils Postpile region

    (Figs. 2, 5), with a locally elevated extracaldera

    heat-flow anomaly (Lachenbruch et al., 1976), and

    with a salient in the local gravity low that extends

    from the caldera as far as 5 km southwest of Mam-

    moth Mountain(Carle, 1988).

    The recent unrest farther east, however, including

    intense seismicity in the calderas south moat and

    renewed uplift of the resurgent dome (Hill et al.,

    2003), is less easily reconciled with the volcanological

    history. With no eruption on the resurgent dome since

    650 ka and no silicic eruption in the south moat since

    f 300 ka, current intrusion of rhyolite there would be

    astonishing. If the inflation source modeled 6 7 km

    beneath the resurgent dome(Langbein, 2003) were amafic dike, it would be the easternmost mafic event

    recognized (inside or outside the caldera) in 2.5 Myr

    and the first evidence for dike penetration through

    much of the crystallizing silicic reservoir. Seismicity

    in the south moat is consistent with displacements on

    reactivated strands of the ring-fault zone (Prejean et

    al., 2002), and eastward advance of a mafic dike along

    that zone would not be unprecedented. The eastern-

    most vent of the western mafic array, perhaps as

    young as 98 ka (Ring, 2000), is merely 3 km south-

    west of Casa Diablo(Fig. 5).Alternative to magmaticintrusion, however, hydrothermal processes may ulti-

    mately be implicated in the current unrest.

    Studies of active and fossil hydrothermal systems

    in Long Valley caldera(Sorey et al., 1991; Goff et al.,

    1991; McConnell et al., 1997; Farrar et al., 2003;

    Fischer et al., 2003; Pribnow et al., 2003)have called

    attention to two separate intervals of hydrothermal

    activity and hot-spring discharge, one ending some-

    time afterf 300 ka and the current one active from

    f 40 ka to the present. The earlier episode ended

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    soon after emplacement of the southeast cluster of

    moat rhyolites, which included the last crystal-poor

    rhyolites ever erupted from the Long Valley reservoir.

    The younger hydrothermal episode started up aboutthe time of eruption of the NW-wall dacite chain (40

    27 ka), which was fed from a reservoir of hybrid

    magma stored beneath the NW moat; and many of the

    studies cited indeed indicate that the active hydrother-

    mal areas in the south moat are supplied by shallow

    aquifers that are fed in turn by deep upwelling

    somewhere in the west moat. Although the 0.65-ka

    Inyo dike probably mixed with the survivingmagmas

    beneath the NW moat, the 7-m-thick dike (Eichel-

    berger et al., 1985) is not itself an adequate heat

    source. No pulse of hydrothermal activity temporally

    related to either the west-moat rhyolites (160100 ka)

    or the Mammoth Mountain silicic pile (11057 ka)

    has been recognized.

    Of the several systems (Fig. 6), the Mono-Inyo

    chain appears to remain magmatically most robust, its

    Holocene activity by far the most vigorous. The Glass

    Mountain rhyolite system is long dead and the Long

    Valley rhyolite reservoir moribund. The Mammoth

    Mountain silicic system appears to have crystallized,

    though renewed mafic activity in its peripheral array

    would not be unexpected. As many as 20 Mono-Inyo

    vents have been active in the last 2000 years, severalof the eruptions have been plinian or subplinian, and

    nearly every batch of Holocene magma erupted has

    been very crystal-poor, implying active separation of

    high-silica melt. At least three times in the Holocene

    (North Deadman dome, Wilson Butte, and the 650-

    year-old Inyo dike), Mono magma has advan