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SpectropolarimetrySpectropolarimetryat THÉMISat THÉMIS
Frédéric Paletou & Guillaume MolodijFrédéric Paletou & Guillaume Molodij
THÉMISVTT
GCT• Latitude : 28°18’ N• Longitude : 16°30’ W• Altitude : 2456 m
THÉMIS:THÉMIS:an overviewan overview
• The telescope & polarimeter
• The transfer optics
• The spectrographs & detectors
PolarimeterPolarimeterlocationlocation
A “unique”A “unique”design!design!
Ritchey-Chrétien pointing directly@ the Sun
With a 90 cm diameter light collector, THÉMIS is the 2nd
largest solar telescope worldwide
Polarization AnalysisPolarization Analysis
The polarimeter is located @ the telescope’s (F1) Cassegrain focus
THÉMIS IS A “POLARIZATION FREE” SOLAR TELESCOPE
M7
M6
M5
M4
F1
TELESCOPE
TRANSFEROPTICS
Entrance window
Secondary mirror
Primary mirror
Polarisation analyserExit window
Focusingtelescope
Tilting mirror
The PolarimeterThe Polarimeter• Consists in 2 achromatic quarter wave plates —
which can be independently rotated over a 45° range, 22.5° stepwise — followed by a calcite beam-splitter
The Quarter Wave PlatesThe Quarter Wave Plates• Cristalline QWPs consisting in a pair of [Quartz + MgF2]
elementary plates (by Optique J. Fichou, France)Phase [degrees]
Wavelength [Å]
The Transfer OpticsThe Transfer Optics
M7
M6
M5
M4
M3
F1
M8 M9
Echelle grating
TRANSFEROPTICS
Primary mirrorExit window
Focusingtelescope
Fieldrotator
F2 Focus
Tilting mirror
Polarisation analyser
• Re-imaging (f/63) • Derotating • Corrections of
chromatisms
The SpectrographsThe Spectrographs
• 1 predisperser (to choose from):
– 79 grooves mm-1 (63º)– 150 grooves mm-1 (2º) – 1200 grooves mm-1 (45º)
• 1 echelle grating:
– 79 grooves mm-1 (63º)
2 in serie:2 in serie:
M7
M3
SP1 MTR
DPSM
IPM
IPM
M8 M9
M6
M7
M10
M11
Echelle grating
OPTICStelescope
Fieldrotator
CCD 3
F2 Focus
CCD 1
CCD 2
Echellespectrograph
Predisperserspectrograph
MS
DP
tra
nsf
er
optic
s
Transfer Transfer optics optics to the to the
detectorsdetectors
• Thomson TH7863Thomson TH7863
• 12 bits12 bits
• 384x288 pixels384x288 pixels
• FW = 8x10FW = 8x1055 e e--
• TTnumnum = 236 ms = 236 ms
Active Regions MagnetometryActive Regions Magnetometry
IIcontinuumcontinuum
BB////
Courtesy Dr N. Meunier, OMP Tarbes (November 25, 2000)
NiI line @ 676.8 nm. The total FOV is 136”x110” and the average seeing was about 0.6” during the scan period
Weak Polarization SignalsWeak Polarization Signals
The enigmatic linear polari-zation of the D2 line of NaI (measured at ~ 0.15).
F. Paletou & G. Molodij (April 7, 2000)
Resonance polarization of the SrI @ 460.7 nm line at the northern limb (and depolariz-ation in the nearby FeI line).
J. Trujillo Bueno et al. (May 29, 2000)
THÉMIS/MTR mode in figuresTHÉMIS/MTR mode in figures• Full-Stokes spectropolarimetry in 6 spectral
domains simultaneously, across a 260 nm range (THEMIS bandpass is ~ 450-900 nm)
• High spatial & spectral resolution (0.5”) & resolving power ~ 300000
• Vector magnetometry: 2’x2’ scans in ~ 10 mn (with a 300 ms exposure time per frame)
• Beam exchange for all the Stokes parameters
• 400-700 nm & 600-900 nm achromatic quarter wave plates available
New in 2001!