CME 20030526
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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 |
20030526.165005.p084g |
16:50 |
95 |
762 |
-22.5 |
2.5e+14 |
No |
Yes |
Table 2 - UVCS Observation Sequence |
FITS filename |
PA (deg) |
T i (UT) |
Tf (UT) |
Height (Rsun) |
Slit W. (arcsec) |
Exp. Time (sec) |
d03.05.26.16:52:27.ovi.dat |
75 |
16:52:49 |
18:40:49 |
1.72 |
27 |
120 |
d03.05.26.18:50:53.ovi.dat |
75 |
18:51:15 |
21:31:15 |
1.75 |
27 |
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) |
d03.05.26.16:52:27.ovi.dat |
1022.20 |
1043.60 |
996.100 |
1001.00 |
|
974.500 |
988.000 |
|
1209.90 |
1222.30 |
|
d03.05.26.18:50:53.ovi.dat |
1024.00 |
1043.20 |
1005.00 |
1013.10 |
|
998.000 |
1002.00 |
|
967.200 |
981.100 |
|
943.400 |
966.300 |
|
1170.70 |
1191.90 |
Table 4 - UV Properties |
First Obs. | Max blue-shift (km/sec) | Max red-shift (km/sec) | Detected at (Rsun) | Lines |
2003/05/26 17:18 | 1.68,1.69 |
HILya1216 CIII977 OVI1032 OVI1038 | ||
Images |
Intensity Images |
H I Lya 1216A intensity image. The Lya line is present just in the first FITS file. |
O VI 1032A intensity image. In the first set of data no significant O VI changes are detected. |
Interpretation |
Front | No |
Void | No |
Shock | No |
Current Sheet | No |
Prominence | Yes |
Flare O VI | ? |
Leg | No |
Helix | No |
Comments |
In the second FITS file, brightening of the O VI lines is detected at the beginnig of the observation. It maybe due to the brightening of the post-CME loops
Last Update Fri Apr 17 22:21:47 2009