CME 20031028

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Table 1 - General Information

CME ID
 Time (UT)
 PA (deg)
 Speed (km/sec)
 Acceleration (m/sec2)
 Mass (g)
 Type II RB
X Flare
20031028.113005.p015s
 11:30
 Halo
 2459
 -105.2*
 4.0e+16*
 No
 Yes


Table 2 - UVCS Observation Sequence

FITS filename
 PA (deg)
 T i (UT)
 Tf (UT)
 Height (Rsun)
 Slit W. (arcsec)
 Exp. Time (sec)
s03.10.28.09:51:58.ovi.dat
 90
 10:54:47
 11:04:47
 1.90
 41
 120

90
 11:07:37
 11:15:37
 1.75
 41
 120

90
 11:17:37
 11:21:37
 1.60
 41
 120
s03.10.28.11:26:37.ovi.dat
 135
 11:27:07
 11:41:07
 3.00
 41
 120

135
 11:44:21
 12:08:21
 2.50
 41
 120

135
 12:11:55
 12:25:55
 2.10
 41
 120

135
 12:29:08
 12:39:08
 1.90
 41
 120

135
 12:41:48
 12:49:48
 1.75
 41
 120

135
 12:51:53
 12:55:53
 1.60
 41
 120
s03.10.28.13:00:51.ovi.dat
 180
 13:01:21
 13:15:21
 3.00
 41
 120

180
 13:18:44
 13:42:44
 2.50
 41
 120

180
 13:46:26
 14:00:26
 2.10
 41
 120

180
 14:03:47
 14:13:47
 1.90
 41
 120

180
 14:16:31
 14:24:31
 1.75
 41
 120

180
 14:26:28
 14:30:28
 1.60
 41
 120
s03.10.28.14:35:28.ovi.dat
 225
 14:35:58
 14:49:58
 3.00
 41
 120

225
 14:53:12
 14:57:12
 2.50
 41
 120

UVCS Slit Position

MOVIE of UVCS Slit on LASCO Images

Table 3 - UVCS Observation Wavelength Range

FITS filename
 Wave Min (A)
 Wave Max (A)
s03.10.28.09:51:58.ovi.dat
 1024.30
 1042.80

967.500
 979.700

1205.90
 1217.00
s03.10.28.11:26:37.ovi.dat
 1024.30
 1042.80

967.500
 979.700

1205.90
 1217.00
s03.10.28.13:00:51.ovi.dat
 1024.30
 1042.80

967.500
 979.700

1205.90
 1217.00
s03.10.28.14:35:28.ovi.dat
 1024.30
 1042.80

967.500
 979.700

1205.90
 1217.00


Table 4 - UV Properties

First Obs. Max blue-shift (km/sec) Max red-shift (km/sec) Detected at (Rsun) Lines
2003/10/28 11:12 2.55,2.10,1.87,1.70,1.51(PA=90), 3.11,2.57,2.13,1.90(PA=135) HILya1216
OVI1032
OVI1038

Images

Intensity Images

HI Lya Intensity Difference at PA=135

HI Lya Intensity at PA=90.

Ovi 1032 Intensity at PA=235

OVI 1032 Intensity at PA=90.


Interpretation

Front Yes
Void No
Shock ?
Current Sheet No
Prominence Yes
Flare O VI No
Leg No
Helix No

Comments

The data show a high background due to the X-ray flare and at 11:12 UT at 1.70R O VI lines are broader. This might indicate the passage of the front. Data show very high background in the panel where O VI, Lyb and Si XII lines are.

Last Update Mon May 7 18:02:53 2012