CME 19990318

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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
19990318.035405.p057s
03:54
60
375
0.8
1.7e+15
No
Yes


Table 2 - UVCS Observation Sequence

FITS filename
PA (deg)
T i (UT)
Tf (UT)
Height (Rsun)
Slit W. (arcsec)
Exp. Time (sec)
d99.03.18.07:12:50.ovi.dat
45
07:14:03
07:19:03
1.50
28
100


07:20:49
07:29:09
1.75
28
100


07:31:04
07:42:44
2.00
28
100


07:44:50
07:59:50
2.25
28
100

UVCS Slit Position

MOVIE of UVCS Slit on LASCO Images


Table 3 - UVCS Observation Wavelength Range

FITS filename
Wave Min (A)
Wave Max (A)
d99.03.18.07:12:50.ovi.dat
1023.20
1043.80

980.400
993.400

1208.70
1220.60

975.800
979.200

1221.80
1224.90


Table 4 - UV Properties

First Obs. Max blue-shift (km/sec) Max red-shift (km/sec) Detected at (Rsun) Lines
1999/03/18 07:14? 0 0 1.45, 1.74, 2.03 HILya1216
OVI1032
OVI1038

Images

Intensity Images

LyA Intensity, background corona not subtracted

OVI 1032 Intensity, background corona not subtracted


Interpretation

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

Comments

CME passed the slit by considering the timing. But it is hard to pick out transient material in the data.

Last Update Tue May 19 11:58:38 2009