Halo CME Mail

Date: Mon, 24 May 2004 11:04

From: Guillermo Stenborg

Subject: 'Full' Halo CME on 2004/05/23, backsided



UCMEO 93001 40524 1505/
40523 61106 82042 0002/ 360// 123// 30693
///// ///// ///// ///// ///// /////
99999

PLAIN

BT


LASCO observed a full halo CME on 2004/05/23. The event was 
first observed in C2 at 11:06 UT developing as a very bright 
ragged loop front above the W limb. Very faint extensions 
are first seen to N at 11:50 UT. By 12:50 UT the C2 occultor 
is completely covered. The front first appeared in C3 images 
at 11:42 UT as a thick and bright ragged loop front above the 
W Limb, the bulk of the ejecta developing toward W. By 15:18 UT 
the C3 occultor is completely covered. By that time, the LE of 
the front on W Limb is already at about 18.5 solar radii. The 
mean plane-of-sky speed for this event at PA 267 was 693 km/s 
(based only in C3 data). For reference, the mean plane-of-sky 
speed at different PA as obtained from C3 measurements is given 
below:

PA 006: 281 km/s
PA 045: 240 km/s
PA 326: 366 km/s

EIT Fe XII running difference images show signatures of a big 
CME coming out from behind the disk, all above the West limb, 
since 11:00 UT. An intensity disturbance is seen to travel 
toward N and S (always above the limb) as the event develops. 
GOES recorded a B4.3 X-ray flare between 11:30 and 11:43 on 
NOAA AR 10618, by the time at S12E32, which most likely has no 
association with the halo event. This event has therefore been 
determined as a 'full' (asymmetric) halo CME, backsided. 

Movies and images of the event will shortly be available at:

ftp://ares.nrl.navy.mil/pub/lasco/halo/20040523

Best wishes,
       
            Guillermo Stenborg

++
Dr. Guillermo A. Stenborg   
SOHO-LASCO Operations Scientist,                                           
CUA, MC 682.3, Bldg 26, Rm 001,   F: +1-301-286-0264         
NASA Goddard Space Flight Center,
Greenbelt, MD 20771.              P: +1-301-286-2941

e-mail: stenborg@kreutz.nascom.nasa.gov
++