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.

C III 977A intensity image.


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