CME 20031118

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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
20031118.095005.p087s
09:50
95
1824
59.6
2.2e+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)
s03.11.18.10:02:39.ovi.dat
90
10:03:14
10:13:14
1.75
41
120

90
10:16:12
10:24:12
1.60
41
120
s03.11.18.10:29:26.ovi.dat
135
10:29:59
10:39:59
1.75
41
120

135
10:42:45
10:50:45
1.60
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)
s03.11.18.10:02:39.ovi.dat
1024.20
1043.10

989.000
993.200

985.400
987.800

1204.10
1206.20

970.600
979.900

1211.30
1219.90
s03.11.18.10:29:26.ovi.dat
1024.20
1043.10

989.000
993.200

985.400
987.800

1204.10
1206.20

970.600
979.900

1211.30
1219.90


Table 4 - UV Properties

First Obs. Max blue-shift (km/sec) Max red-shift (km/sec) Detected at (Rsun) Lines
2003/11/18 10:03 115 1.70,1.53 (PA=90); 1.73,1.55 (PA=135) HILya1216
HILyb1026
CIII977
OVI1032
OVI1038
SiIII1207
NIII990

Images

Intensity Images

H I Lya 1216A intensity image at PA=135

O VI 1032A intensity image at PA=135

O VI 1032 A intensity image at PA=90

H I Lya intensity image at PA=90. The gap in Lya at 1.70R is intepreted as evidence for the presence of a current sheet (see comments).


Interpretation

Front ?
Void ?
Shock ?
Current Sheet Yes
Prominence Yes
Flare O VI ?
Leg ?
Helix ?

Publications

Lin J. et al. 2005, ApJ,662,1251

Comments

The gap in H I Ly-alpha image at 1.70 R (PA=90) that gradually disappeared as result of the reconnection inflow near the current sheet

Last Update Thu May 10 14:40:43 2012