cor2 status - nasa · 2007. 3. 29. · instrument status 5th secchi team meetiing.2 • fm-a first...

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5 th SECCHI Tam Meeting.1 COR2 Status Angelos Vourlidas

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Page 1: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

5th SECCHI Tam Meeting.1

COR2 Status

Angelos Vourlidas

Page 2: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Instrument Status

5th SECCHI Team Meetiing.2

• FM-A first light on Dec 4, 2006• FM-B first light on Dec 13, 2006.• Both telescopes are functioning nominally.• The only issue is the boresight offset.

– Both telescopes are offset from Sun center by > ~ 2 arcminutes.– COR2B is most affected because STEREO-B is in perihelion.– This problems has slowed down COR2 commissioning

activities.• Small amount of jitter seen around the occulter.

HOWEVER,• The overall data quality is great.

Page 3: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Commissioning Status

5th SECCHI Team Meetiing.3

• Calibrations Completed– Light leak– CCD linearity, dark current, binning modes, compression– Exposure time stability, accuracy– Pointing checks (offpoints from nominal)– Polarization calibration (15 deg step, S/C rolls)– Thermal run (for focus check)– Spatial Resolution

• Calibrations Pending– Photon transfer curve (PTC)– MTF using stars– Stay light (deep exposures)– Pointing (sun center, rel to SCIP instruments).

Page 4: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Offpoint – COR2B

5th SECCHI Team Meetiing.4

• Stray light is more prominent in FM-B because the S/C is not at its proper distance from the Sun yet.

Page 5: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Offpoint – COR2A

5th SECCHI Team Meetiing.5

• Stray light is not a serious ptoblem in FM-A

Page 6: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Early Observations

5th SECCHI Team Meetiing.6

• Typical cadence : 2 hrs• Typical image: pB sequence (images at 0, 120 , 240 deg) • Sequence duration: 24 sec• Typical size: 2048x2048 (Full resolution)• Spatial Resolution: 14.7 arcs/pix• Observed CMEs, Comets, plumes

SCIENCE TEAM• Angelos Vourlidas, D. Socker, S. Plunkett, C. Korendyke, S.

Patsourakos• A. Thernisien, R. Colaninno

Page 7: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

First Light- COR2A

5th SECCHI Team Meetiing.7

%Polarization Total Brightness

Page 8: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Comparison w/ LASCO

5th SECCHI Team Meetiing.8

Page 9: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Moon Transit

5th SECCHI Team Meetiing.9

Page 10: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Backup Slides

5th SECCHI Team Meetiing.10

Page 11: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

Summary

5th SECCHI Team Meetiing.11

Parameter Required Performance

Measured Performance

FOV (deg) 8 8.4

Polarization Accuracy 10% 2%

Min. Vignetting 80% 80%

Nominal Exposure (sec) 4 4

Spatial Resolution (arcsec) 30 25-30

FWHM Bandpass (nm) 650-750 650-770

Stray Light @ 6Rsun (MSB) < 2·10-10 < 3·10-11

Page 12: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

COR2 Spectral Calibration

5th SECCHI Team Meetiing.12

• Calibration based on LASCO’s Lightboxusing new Spectrometer.

• Accuracy ~20%.

SRIPS FWHM

Page 13: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

COR2-A Stray Light Details

5th SECCHI Team Meetiing.13

Page 14: COR2 Status - NASA · 2007. 3. 29. · Instrument Status 5th SECCHI Team Meetiing.2 • FM-A first light on Dec 4, 2006 • FM-B first light on Dec 13, 2006. • Both telescopes are

COR2 Vignetting

5th SECCHI Team Meetiing.14

COR2-A Vignetting Function. Contours at 10% intervals. Inner contour is 10%.