CME 20031026

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
20031026.175405.p235s
 17:54
 270
 1537
 4.8
2.0e+16*
 No
 Yes


Table 2 - UVCS Observation Sequence

FITS filename
 PA (deg)
 T i (UT)
 Tf (UT)
 Height (Rsun)
 Slit W. (arcsec)
 Exp. Time (sec)
d03.10.26.16:39:53.ovi.dat
 245
 17:33:31
 20:33:31
 2.00
 13
 600
d03.10.26.20:39:35.ovi.dat
 246
 20:40:56
 02:40:56
 2.40
 20
 600
s03.10.27.03:27:44.ovi.dat
 270
 03:28:38
 03:42:38
 3.00
 41
 120


03:45:58
 04:09:58
 2.50
 41
 120


04:13:35
 04:27:35
 2.10
 41
 120


04:31:00
 04:41:00
 1.90
 41
 120


04:43:40
 04:51:40
 1.75
 41
 120


04:53:45
 04:57:45
 1.60
 41
 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)
d03.10.26.16:39:53.ovi.dat
 1028.00
 1043.00

997.200
 1000.70

980.600
 990.600

1211.10
 1220.30

975.900
 979.300

1221.50
 1224.60
d03.10.26.20:39:35.ovi.dat
 1028.00
 1043.00

997.200
 1000.70

980.600
 990.600

1211.10
 1220.30

975.900
 979.300

1221.50
 1224.60
s03.10.27.03:27:44.ovi.dat
 1024.30
 1042.80

967.500
 979.700

1205.90
 1217.00


Table 4 - UV Properties

First Obs. Max blue-shift (km/sec) Max red-shift (km/sec) Detected at (Rsun) Lines
2003/10/26 17:33 350 2.01, 2.46 (PA=245,246); 3.10,2.56,2.11,1.88,1.71 (PA=270) HILya1216
OVI1032
OVI1038

Images

Intensity Images

H I Lya 1216A intensity image at 2.46 R

H I Lya 1216A intensity image at 1.66 and 2.01R

H I Lya 1216A intensity image during the synoptic scan at PA=270. A narrow feature is detected.

O VI 1032A intensity image at 1.66 and 2.01R

UV spectra from 17:27 to 19:06 UT showing the evolution on the spectral lines as the CME passes through the UVCS slit. The high background is caused to the X-ray flare.


Interpretation

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

Comments

The spectra during the passage of the front are taken with 600sec exposure time.

Last Update Wed May 13 21:30:44 2009