CME 19990402
Tutorials: UVCS CME Observations pdf / html | UVCS CME Catalog Pages html |
Table 1 - General Information |
CME ID |
Time (UT) |
PA (deg) |
Speed (km/sec) |
Acceleration (m/sec2) |
Mass (g) |
Type II RB |
X Flare |
19990402.083005.p079s |
08:30 |
90 |
1068 |
-21.3 |
2.4e+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) |
d99.04.02.08:10:43.ovi.dat |
45 |
08:11:14 |
08:17:54 |
1.50 |
28 |
200 |
08:18:38 |
08:25:18 |
1.60 |
28 |
200 | ||
45 |
08:26:08 |
08:35:08 |
1.70 |
28 |
180 | |
08:37:13 |
08:46:13 |
1.90 |
28 |
180 | ||
45 |
08:48:12 |
09:00:12 |
2.10 |
28 |
180 | |
09:02:23 |
09:17:23 |
2.50 |
28 |
180 | ||
45 |
09:20:28 |
09:42:28 |
3.00 |
28 |
200 | |
d99.04.02.09:49:21.ovi.dat |
90 |
09:49:53 |
09:56:33 |
1.50 |
28 |
200 |
09:57:17 |
10:03:57 |
1.60 |
28 |
200 | ||
90 |
10:04:40 |
10:13:40 |
1.70 |
28 |
180 | |
10:15:38 |
10:24:38 |
1.80 |
28 |
180 | ||
90 |
10:26:38 |
10:38:38 |
2.00 |
28 |
180 | |
10:40:51 |
10:55:51 |
2.30 |
28 |
180 | ||
90 |
10:58:53 |
11:24:13 |
2.80 |
28 |
200 | |
11:27:02 |
12:01:42 |
3.50 |
28 |
200 |
UVCS Slit Position | MOVIE of UVCS Slit on LASCO Images |
Table 3 - UVCS Observation Wavelength Range |
FITS filename |
Wave Min (A) |
Wave Max (A) |
d99.04.02.08:10:43.ovi.dat |
1023.20 |
1043.70 |
980.400 |
993.400 |
|
1208.70 |
1220.60 |
|
975.800 |
979.200 |
|
1221.80 |
1224.90 |
|
d99.04.02.09:49:21.ovi.dat |
1023.20 |
1043.70 |
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 |
1999/04/02 08:22 | 89 | 136 | 1.43,1.55,1.67,1.78,1.9,2.0,2.1,2.35,2.58,3.1,3.6 |
HILya1216 HILyb1026 CIII977 OVI1032 OVI1038 OV1218 |
Images |
Intensity Images |
Plots and more |
Interpretation |
Front | No |
Void | ? |
Shock | No |
Current Sheet | No |
Prominence | Yes |
Flare O VI | No |
Leg | ? |
Helix | ? |
Comments |
The Doppler shifts of 2 blobs at 1.67 and 1.90 Ro of the PA=45 observations show changing shift from one to the next exposure, indicating possible helical motion. However, since this only occurs in two exposures in the available data, existence of helix or not can not be definitely certain.
Last Update Wed May 9 16:05:13 2012