| Direct Image | Subtraction Image |
|---|---|
|
|
| 18:00 UT | 18:00 minus 17:40 |
This event became visible in the MK3 instrument at around 17:48 UT and left at
approximately 18:09 UT. The event was travelling southward throughout the MK3
measurements, explaining the large difference in position angle of the
beginning of the event from the end.
The event became visible in the
LASCO
C2 field of view at approximately 18:27 UT (at least that was the first C2
image available for measurements.) The outer loop feature became
distorted here and it became difficult to identify a cavity feature. For this
reason, there are no cavity measurements in the LASCO C2 fields of view. The
event was not really visible in the C3 field of view.
Here are the preliminary LASCO notes for this event. There were two events visible on this day in C2, the first one is a very bright event on the eastern limb early in the day. The second, and the one corresponding to this MK3 event, was observed later in the day on the west limb.
There is a MK3 direct-image movie [GIF, 964K] and a MK3 subtraction movie [GIF, 854K] to view for this event.
There is also a LASCO C2 movie [MPEG, 323 KB] of this event.
There were a total of 28 data points obtained for use in trajectory fits.
Of those, 12 were for the outer loop, 7 for the cavity, and 9 for the core
feature.
The event times were from 17:48UT
until 20:55 UT.
The event was visible in MK3 and continued past the LASCO C2 field of view.
Central Position Angle: ~265 - Loop (in degrees) ~265 - Cavity ~260 - CoreThe following data is obtained from performing a second order, least squares fit of the trajectory data points (Hundhausen, et al, 1994) :
Width (degrees): ~43 - Loop (MK3) ~21 - Cavity (MK3) ~11 - Core (MK3)
Start Times (UT): 17:35:05 - Loop 17:38:16 - Cavity 17:39:57 - Core Start Heights (Solar Radii): 1.0 - Loop 1.0 - Cavity 1.9 - Core Final Speeds (km/s): 248.5 - Loop (out to C2) 313.1 - Cavity (out to C2) 224.5 - Core (out to C2) Accelerations (km/s^2): -0.05 - Loop 0.03 - Cavity 0.03 - CoreThe above numbers were produced from a second-order fit of trajectory data which began in MK3 and ended in LASCO C3. Estimated start times, start heights, final speeds and accelerations are available in each individual data set (MK3, C2, and C3) where enough data points were available. That information is not presented here. Final speeds were evaluated at last data point in C3 except where noted.
| First Order | Second Order |
|---|---|
| (Loop, Cavity, & Core) | (Loop, Cavity & Core) |
|
|
| MK3 and C2 | MK3 and C2 |
A gallery of the `best' direct and the `best' subtraction images (`display' version) from this event may be accessed below.
Be aware that these are only a few of the images that you may access. For a complete list of images, including the `computational' versions, please visit our FTP site.
All times are given in Universal Time (UT) units.
Best MK3 Direct Images
MK3 images :
Best MK3 Subtraction Images
MK3 images :
Hundhausen, A.J., J.T. Burkepile, and O.C. St.Cyr, Speeds of coronal mass ejections: SMM Observations from 1980 and 1984-1989, J. Geophys. Res., 99, 6543-6552, 1994.
Return to the MLSO CME
home page