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Magnetospheric solitary structure maintained by 3000 km/s ions as a cause of westward moving auroral bulge at 19 MLT M. Yamauchi 1 , I. Dandouras 2 , P.W. Daly 3 , G. Stenberg 4 , H. Frey 5 , P.-A. Lindqvist 6 , Y. Ebihara 7 , R. Lundin 1 , H. Nilsson 1 , H. Reme 2 , M. Andre 4 , E. Kronberg 3 , and A. Balogh 8 (1) IRF, Kiruna, Sweden, (2) CESR, Toulouse, France, (3) MPS, Katlenburg-Lindau, Germany, (4) IRF, Uppsala, Sweden, (5) UCB/SSL, Berkeley, CA, USA, (6) Alfvén Lab., KTH, Stockholm, Sweden, (7) IAR, Nagoya U., Nagoya, Japan, (8) Blackett Lab., ICL, London, UK Cluster workshop, 2009-5-15

Cluster workshop, 2009-5-15

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Page 1: Cluster workshop, 2009-5-15

Magnetospheric solitary structure maintained by 3000 km/s ions as a cause of westward moving auroral

bulge at 19 MLTM. Yamauchi1, I. Dandouras2, P.W. Daly3, G. Stenberg4, H. Frey5, P.-A. Lindqvist6, Y. Ebihara7, R. Lundin1, H. Nilsson1, H. Reme2, M. Andre4, E. Kronberg3, and A. Balogh8

(1) IRF, Kiruna, Sweden, (2) CESR, Toulouse, France, (3) MPS, Katlenburg-Lindau, Germany, (4) IRF, Uppsala, Sweden, (5) UCB/SSL, Berkeley, CA, USA, (6) Alfvén Lab., KTH, Stockholm, Sweden, (7) IAR, Nagoya U., Nagoya, Japan, (8) Blackett Lab., ICL, London, UK

Cluster workshop, 2009-5-15

Page 2: Cluster workshop, 2009-5-15

* Z ≈ 0 RE

* 60 GMLat

* 19 MLT

S/C

sun

tail

Cluster Perigee

Page 3: Cluster workshop, 2009-5-15

IMAGE(FUV)

ions ≈ 3000 km/s

ions > 5000 km/s

0.01~40 keV

P/A

P/A

overview

06:42 06:46 06:4806:44

Page 4: Cluster workshop, 2009-5-15

Sudden change in fieldExB (>50 km/s) is observede.g., 57 km/s : He+ ~ 70 eV H+ ~ 17 eV

Page 5: Cluster workshop, 2009-5-15

Timing (B ≠ E)

(1) single peak of E: lead by SC-3 by 1~10 sec

(2) Pi2-like rarefaction of B: simultaneous at all SC

propagate

Page 6: Cluster workshop, 2009-5-15

Timing from ExB convection

SC-3 leads against SC-1 by 10 sec: agree with field data

Page 7: Cluster workshop, 2009-5-15

Timing Sunward propagation of E& E is nearly // to Propagation direction

1000~2000 km

Page 8: Cluster workshop, 2009-5-15

06:43 UT event (arrival of auroral bulge)

(a)Sunward propagation (5~10 km/s) of DC field * depletion of |B|≈BZ up to 25%

* polarization E≈-EX of up to 10 mV/m

* ExB convection (up to 50 km/s) of cold He+ (without O+)

Page 9: Cluster workshop, 2009-5-15

increase in ion flux

decrease in ion flux

H+ < 90 keV

H+ > 160 keV

Page 10: Cluster workshop, 2009-5-15

increase in ion flux

decrease in ion flux

He < 350 keV

He > 700 keV

O < 0.9 MeV

O > 1.4 MeV

Page 11: Cluster workshop, 2009-5-15

All relevant ion channel

3000 km/s = 50 keV (H), 190 keV (He), 740 keV (O)5000 km/s = 130 keV (H), 500 keV (He), 2 MeV (O)

Page 12: Cluster workshop, 2009-5-15

06:43 UT event (arrival of auroral bulge)

(a) Sunward propagation (5~10 km/s) of DC field * depletion of |B|≈BZ up to 25%

* polarization E≈-EX of up to 10 mV/m

* ExB convection (up to 50 km/s) of cold He+

(b) Net flux Increase of selectively 3000 km/s ions* ∆P3000km/s = 3 nPa = - ∆PB. * net decrease of other energetic particles.

Page 13: Cluster workshop, 2009-5-15

Drift motionVB energy (mass independent)

VExB = constant (energy mass)

50 keV H+ drift = 15 km/s190 keV He+ drift = 60 km/s740 keV O+ drift = 220 km/s

Simultaneous appearance & much faster than the motion of the E-structure a solitary structure to maintain the flux peak

Page 14: Cluster workshop, 2009-5-15

ion-scale ?gradient is less than 500 km (5~10 km x 50 sec)

cf. RB (= mv/qB) for B ≈ 200 nT condition

50 keV 200 keV 1 MeV

H+ v = 3000 km/s

RB = 150 km

v = 6000 km/s

RB = 300 km

v = 14000 km/s

RB = 700 km

He+ v = 1500 km/s

RB = 300 km

v = 3000 km/s

RB = 600 km

v = 7000 km/s

RB = 1400 km

O+ v = 700 km/s

RB = 600 km

v = 1500 km/s

RB = 1200 km

v = 3500 km/s

RB = 3000 kmRB(H+) ≤ gradient ≤ RB(He+) << RB(O+)

Page 15: Cluster workshop, 2009-5-15

06:43 UT event (arrival of auroral bulge)

(a) Sunward propagation (5~10 km/s) of DC field * depletion of |B|≈BZ up to 25%

* polarization E≈-EX of up to 10 mV/m

* ExB convection (up to 50 km/s) of cold He+

(b) Net flux Increase of selectively 3000 km/s ions* ∆P3000km/s = 3 nPa = - ∆PB. * net decrease of other energetic particles. * propagating solitary structure.* scale size ~ gyro radius

Page 16: Cluster workshop, 2009-5-15

IMAGE(FUV)

ions ≈ 3000 km/s

ions > 5000 km/s

0.01~40 keV

P/A

P/A

overview

06:42 06:46 06:4806:44

Page 17: Cluster workshop, 2009-5-15

At around 06:44 UT, appearance of 7 keV // O+ from both hemisphere, within 40 sec difference

// keV ion

Page 18: Cluster workshop, 2009-5-15

06:43 UT event (arrival of auroral bulge)

(a) Sunward propagation (5~10 km/s) of DC field * depletion of |B|≈BZ up to 25%

* polarization E≈-EX of up to 10 mV/m

* ExB convection (up to 50 km/s) of cold He+

(b) Net flux Increase of selectively 3000 km/s ions* ∆P3000km/s = 3 nPa = - ∆PB. * Net decrease of other energetic particles.* propagating solitary structure.* scale size ~ gyro radius

(c) Conjugate with auroral bulge* Parallel O+ of ≈ 7 keV is detected

Page 19: Cluster workshop, 2009-5-15

Cluster observed westward moving auroral bulge at 19 MLT on 2002-5-19 is caused by a solitary structure in the magnetosphere.

The solitary structure consists of polarization E-field (up to 10 mV/m) and depletion of B≈Bz.

This solitary structure is maintained by energetic ions of 3000 km/s speed for all ions.

Size (gradient < 500 km) of this solitary structure is comparable to the ion gyro radius of carrier ions.

conclusion1000~2000 km

Page 20: Cluster workshop, 2009-5-15

End

Page 21: Cluster workshop, 2009-5-15

Many other interesting topics

(1) Qualitative inter-SC difference

(2) Inter-SC time-of-flight examination

(3) Decoupling technique of different plasma using conservation of magnetic moment

Page 22: Cluster workshop, 2009-5-15

Qualitative difference within Rgyro

Distribution function Difference cannot be explained by the slight difference in effective energy between SC.

RB >> inter-SC distance cannot be due to finite gyroradius effect.

gradient is substantially large?

Page 23: Cluster workshop, 2009-5-15

TOF (7 keV O+ = 250 km/s & SC-1 -100km- SC-4 -150km- SC-3)or Phase-angle dependence?

TOF effect or phase effect?

Page 24: Cluster workshop, 2009-5-15

TOF (7 keV O+ = 250 km/s) SC-1/SC-4/SC-3 = 100 km/150 kmor Phase-angle dependence?

Page 25: Cluster workshop, 2009-5-15
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Energy-time dispersion (flux increase)

time-of-flight? (No) ∆T ~ 10 sec for ∆VD ~ 10 km/s source < 1000 km No

finite gyroradius? (Yes) ∆T ~ 10 sec for ∆RB ~ 100 km agree with propagation

VDB = 20~30 km/s

VDB = 10~20 km/s

VDB = 30~50 km/s

VDB = 50~100 km/s

Page 27: Cluster workshop, 2009-5-15

Energetic electron vs B

observed flux

Synchronize with B field variation

|B|

Page 28: Cluster workshop, 2009-5-15

µB = W/B conserved? not really

increasing flux

under µB = const df(µB) = 0

(∂f/∂W)B > 0 (∂f/∂B)W > 0

= real

Page 29: Cluster workshop, 2009-5-15

Linear decoupling

observed flux after decoupling the conservation of µB = W/B

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End

Page 31: Cluster workshop, 2009-5-15

Westward surging aurora

Akasofu et al., 1966

Fujii et al., 1994

= strong upward FAC

Page 32: Cluster workshop, 2009-5-15

conclusion - continuedThe 3000 km/s ions are the main carrier of the propagating diamagnetic current that caused the magnetic depletion propagating sunward.

The sunward propagation of this solitary structure caused the sunward propagation of field-aligned potential drop and hence of the auroral bulge.

Page 33: Cluster workshop, 2009-5-15

sunward propagation

E

prof

ile

Page 34: Cluster workshop, 2009-5-15

Global condition: minor storm Dst ≈ -60 nT

Page 35: Cluster workshop, 2009-5-15

3000 km/s

> 5000 km/s

0.01~40 keV

overview

P/A

P/A

Page 36: Cluster workshop, 2009-5-15

IMAGE/FUV 06:26~06:56 UT

06:26 UT

06:28 UT

06:30 UT

06:32 UT

06:34 UTS/C

06:36 UT

06:38 UT

06:40 UT

06:42 UT

06:44 UT

06:46 UT

06:48 UT

06:50

06:52

06:54

06:56

~06:43 event

Page 37: Cluster workshop, 2009-5-15

AE and Bx

1. Main phase of minor storm (Dst ~ -60 nT).

2. Substorm onset at around 06:25 UT but ceased in ~10 min.

3. New activity started at around 06:38 UT.

4. Aurora bulge arrived Cluster’s conjugate ~19 MLT at around 06:42~06:44 UT.

Page 38: Cluster workshop, 2009-5-15

ion-scale ?All SC should observe the same behavior of ions if ion gyro-radius (RB = mv/qB) >> inter-S/C distance

RB for B ≈ 200 nT condition

10 keV 100 keV 1 MeV

H+ v = 1400 km/s

RB = 70 km

v = 4000 km/s

RB = 200 km

v = 14000 km/s

RB = 700 km

He+ v = 700 km/s

RB = 140 km

v = 2000 km/s

RB = 400 km

v = 7000 km/s

RB = 1400 km

O+ v = 350 km/s

RB = 300 km

v = 1000 km/s

RB = 800 km

v = 3500 km/s

RB = 3000 km

Page 39: Cluster workshop, 2009-5-15

µB conservation: W W//, but

06:43

Page 40: Cluster workshop, 2009-5-15

consolation

S/C distance ≈ 100 km in z direction & 50 km in x-y direction

≈ RB for 10~20 keV H+ << RB for Ring current ions

H+ > 20 keV (O+ > 2 keV) should behave the same at all SCs if the gyrotropic assumption is correct

Page 41: Cluster workshop, 2009-5-15

06:43 UT event (arrival of auroral bulge)

(a) Sunward propagation (5~10 km/s) of DC field * depletion of |B|≈BZ up to 25%

* polarization E≈-EX of up to 10 mV/m

* ExB convection (up to 50 km/s) of cold He+ (without O+)

(b) Net flux Increase of selectively 3000 km/s ions (∆P3000km/s = 3 nPa = - ∆PB).

* Net flux decrease of other energetic particles. * Energy-time dispersion* 100 keV H+ ~ ∆E, and 50 keV H+ ~ ∆B

(c) Ionospheric plasma that is accelerated by parallel potential of about 7 kV.

Page 42: Cluster workshop, 2009-5-15

But, there is inter-SC difference

RAPID (SSD) data

Page 43: Cluster workshop, 2009-5-15

How about CIS (MCP) data?

Page 44: Cluster workshop, 2009-5-15

Inter-SC difference: trapped H+ for CIS

Page 45: Cluster workshop, 2009-5-15
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For flux increase: (1) SC-2 < SC-1 < SC4=SC3

H+: 80~160 keVHe+: 200~300 keV

(2) SC-2 > SC-1 > SC4=SC3H+: ~60 keV O+: 500~600 keV

For flux decrease: (3) SC-2 < SC-1 < SC4=SC2

He+: 400~700 keV(4) SC-2 > SC-1 > SC4=SC3

O+: ~400 keV

inter-SC difference !

Hybrid: (5) SC-2 > SC-1 > SC4 > SC3

O+: 400~500 keV

Page 48: Cluster workshop, 2009-5-15

End

Page 49: Cluster workshop, 2009-5-15

no wave@06:43 UT, wave@06:48 UT

ion

dE

dB

S//

E/B

dBZ

dBXstagnant

BB-EM

spin effects

150 nT ΩP = 4 Hz

ΩHe?

Page 50: Cluster workshop, 2009-5-15

Composition from energy ratio(1) From energy peak: plasmaspheric He+ rich

= 0°

= 180°

= 360°

10 100 [eV] 10 100 [eV]

Precursor (06:44 UT) Heating (06:49 UT)

H+ He+ O+

ratio=4: O+/He+ or He+/H+

18eV 70eVH+ He+

//

//

Page 51: Cluster workshop, 2009-5-15

End

Page 52: Cluster workshop, 2009-5-15

Ground conj.

06:43 06:48

Nothing special

only 50 nT activity