SOHO/LASCO Halo CME  20120512

COMMENTS: HALO CME from Sigmoidal region [S16,E15] resulting from an eruptive filament of the region.
                          LASCO velocity:  961.7 km/sec at PA117 degrees.  Acceleration: 8.13 m/sec^2.

Halo Alert: halo-message.20120512


SOHO/LASCO HALO CME 120512

UCMEO 93001 20516 1920/
20512 60000 80630 1171/ 116// 213// 30962
20511 62318 80051 21516 ///// 2212/
99999

PLAIN

SOHO/LASCO observed a HALO CME on May 12, 2012.  Event is first seen in C2 at
00:00 UT with a wide faint loop surfacing along the east. The loop expands
with extensions to a full halo by 00:36 UT.  A bright loop with core is seen
over the equatorial east area.  This is a separate part of the associated loop system.
The event continues into the C3 field beginning 00:30-06:30 UT out to the edge of field
at 30 Rsun in the SE.

Time/height measurements were marked at 4 points in C2 with speeds of 922.4 Km/sec
at position angle 118 degrees. The event is marked to 7 points in C3.  Speeds
average through both fields to 961.7 Km/sec at PA 118 degrees. Acceleration of
8.13 m/sec^2.

SDO AIA 193 shows activated loops of a region in the SE with sigmoidal properties
located at [S16,E15]. Beginning 23:24 UT, a dimming of the area with flaring and arcade.
AIA 304 shows a filament eruption of the region 23:18-00:51 UT with ejecta from
the northern edge of the region.

STEREO: HR data
COR2 B,  23:53-02:24 UT, a loop expanding over the west.
Preliminary time/height measure gives 1083.4 km/sec velocity at LE.
EUVI B 195, 22:50 UT loops over limb activate and erupt by 23:15-00:10 UT.
EUVI B 304, 23:11-00:31 UT filament material eruption off the west limb.
COR2 A, 23:54-03:24 UT shows an asymmetric halo east.
Preliminary time/height measure gives 727.7 km/sec velocity at LE.
EUVI A 195, 23:05 UT Activated loops which erupt 23:20-23:55 UT. A 2nd emission
north beginning 00:55-01:20 UT which seems associated.
EUVI A 304, 23:26-00:56 UT, CME off east limb.

NOAA reports a flare 23:41-00:01 UT from location [S17,E14]

The observation of this event is considered 'FAIR'. This CME is determined FRONTSIDED.

Images and movies and time/height information for this event is available on the web at:

http://umbra.nascom.nasa.gov/lasco/observations/halo/2012/120512/

Best regards,

Kevin Schenk
Solar Heliospheric Observatory
EIT and LASCO Operations
NASA-Goddard Space Flight Center, USA

BT





SOHO/LASCO C2 Diff
SOHO/LASCO C3 Diff
SDO/AIA 193
20120512_003605_c2rdiff.gif
20120512_014205_c3rdiff.gif
20120511_232707_aia_193.gif
SOHO/LASCO C2
SOHO/LASCO C3
SDO/AIA 304
20120512_014205_c3rdiff.gif
20120512_0142_c3.gif
20120512_000908_aia_304.gif
STEREO/COR2 BEHIND
SDO/AIA 193 DIFF
STEREO/COR2 AHEAD
20120512_012421_cor2_behind.gif
20120511_232707_aia_193_diff.gif
20120512_012400_cor2_ahead.gif
STEREO/EUVI 195 BEHIND
STEREO/EUVI 304 BEHIND
STEREO/EUVI 195 AHEAD
20120511_232551_euvi_195_behind_diff.gif
20120511_232636_euvi_304_behind.gif
20120511_233030_euvi_195_ahead_diff.gif





Time/Height Velocities and Plots

C2/C3
20120512_c2c3_ht.gif

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MPEG Movies



LASCO Software IDL Save Files (.mvi)






  • Please, send questions and comments to Kevin Schenk