CME 20040713

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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
20040713.005405.p213s
00:54
313
607
-2.2*
1.8e+14
Yes
Yes


Table 2 - UVCS Observation Sequence

FITS filename
PA (deg)
T i (UT)
Tf (UT)
Height (Rsun)
Slit W. (arcsec)
Exp. Time (sec)
d04.07.12.23:48:23.ovi.dat
305
23:48:53
00:48:53
2.58
41
50


00:54:13
01:54:13
2.73
41
50
d04.07.13.02:02:30.ovi.dat
340
02:03:00
03:02:10
1.85
41
50


03:08:20
04:08:20
1.93
41
50


04:13:40
05:13:40
2.06
41
50

Table 3 - UVCS Observation Wavelength Range

FITS filename
Wave Min (A)
Wave Max (A)
d04.07.12.23:48:23.ovi.dat
970.900
976.700

1211.60
1216.90
d04.07.13.02:02:30.ovi.dat
970.900
976.700

1211.60
1216.90


Table 4 - UV Properties

First Obs. Max blue-shift (km/sec) Max red-shift (km/sec) Detected at (Rsun) Lines
2004/07/13 01:50 474 22 2.71, 1.70, 1.80, 1.95 HILya1216

Images

Intensity Images

LyA intensity, background corona not subtracted

LyA intensity, background corona not subtracted


Plots and more

Sample expsoure showing large blue shift in LyA

Sample exposure showing complicated structure and line shift

Sample exposure showing complicated structure and line shift

Sample expsoure showing complicated structure and line shift

Sample exposure showing compicated structure and line shift


Interpretation

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

Comments

Some of the 2.71 Rs exposures can be C III too. Care should be taken when ananlyzing the data to identify which blob comes from which line emission.

Last Update Fri Feb 6 19:23:38 2009