sumer observations of comet ison during perihelion · comet ison: dust brightness sharp drop of...
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![Page 1: SUMER observations of comet ISON during perihelion · Comet ISON: Dust Brightness Sharp drop of dust production ~ 0.5 days before perihelion - spike coma with brightness decrease](https://reader033.vdocuments.us/reader033/viewer/2022060907/60a1a04f8cb24229ca5a87f6/html5/thumbnails/1.jpg)
Solar Group Seminar Curdt, February 18 1
SUMER observations of comet ISON during perihelion
Werner Curdt & co-workersMax-Planck-Institut für Sonnensystemforschung
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Solar Group Seminar Curdt, February 18 2
foto taken Nov 12courtesy M. Jäger
Outline• prologue• approach phase• perihelion passage
- observations- results
• post encounter and outlook
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Solar Group Seminar Curdt, February 18 3
foto taken Nov 15courtesy D. Peach
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Solar Group Seminar Curdt, February 18 4
CIOC lightcurve, update on Nov 27
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Solar Group Seminar Curdt, February 18 5
enhanced image of Nov 16 showing wingscourtesy HBO
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Solar Group Seminar Curdt, February 18 6
foto taken Nov 22courtesy F.-H. Hemmerich
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Solar Group Seminar Curdt, February 18 7
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Solar Group Seminar Curdt, February 18 8
accessible FOVimaged areapredicted trajectory
encounter geometry
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Solar Group Seminar Curdt, February 18 9
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Solar Group Seminar Curdt, February 18 10
LASCO C2 imagestaken on Nov 28
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Solar Group Seminar Curdt, February 18 11
slot image in Ly-α scattered light
200 arsec
24
0 arcsec
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Solar Group Seminar Curdt, February 18 12
cometary dust tail at a cadence of 30 s+ predicted nucleus position⋅⋅⋅⋅ trajectory
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Solar Group Seminar Curdt, February 18 13
dust tail details
+ predicted nucleus position
⋅⋅⋅⋅ tail bisector
⋅⋅⋅⋅ trajectory (30 s steps)
↑ vector to Sun center
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Comet ISON: Dust Synchrones & Syndynes
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Comet ISON: Dust Brightness
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Comet ISON: Dust Brightness
Sharp drop of dust production ~ 0.5 days before perihelion- spike coma with brightness decrease in motion direction- PA ~ 65 deg (model) compared to PA ~71 deg (SUMER)- nucleus is not in dust cloud- dust cloud is offset from nucleus trajectory- dust cloud has asymmetric brightness profile
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Solar Group Seminar Curdt, February 18 17
Ly-α profile, disk average composite Ly-α irradiance at 1 AU (LISIRD): 6.24 mW/m2
tail radiance (brighter sections): 24 mW/(m2 sr)
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Solar Group Seminar Curdt, February 18 18
selected spectral windows in spectral mode:
1167 … 1175 / 1199 … 1207 He II, C III, Si II, Si III, H-H1049 … 1055 / 1078 … 1088 O I, N II, CO1036 … 1045 / 1069 … 1077 C II, O VI, Si IV,1301 … 1310 / 1333 … 1341 O I, O I, O I, Si II, CII
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Solar Group Seminar Curdt, February 18 19
courtesy CIOC
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Comet ISON: Dust Synchrones at Perihelion
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Solar Group Seminar Curdt, February 18 21
image taken Dec 18courtesy HST