| Direct Image | Subtraction Image |
|---|---|
|
|
| 19:54 UT | 19:54 minus 19:20 |
This event began around 19:34UT. It contains a classic LOOP/CAVITY/CORE
configuration, each of which were easily measured throughout the MK3 field
of view and out through the
LASCO
C3 field of view.
The above images show both the direct calibrated MK3 image taken
from the K-Coronameter and the same image which has had a pre-event frame
subtracted from it to extract more detail.
The outer loop is visible in both frames. In the subtraction image, the loop
is a bright yellow. The leading edge of the cavity was defined for the
purposes of these trajecotry measurements to be the trailing edge of the outer
loop. This is usually indicated by a depleted region following the loop.
The prominence material, or core, is usually visible as red in the subtractions
and can be seen in the direct image above as a faint, white, dense region
following the loop.
There is a MK3 direct-image movie [GIF, 664K] and a MK3 subtraction movie [GIF, 700K] to view for this event.
There is also a LASCO C2 movie [MPEG, 302 KB] and a LASCO C3 movie [MPEG, 238 KB] of this event as well.
There were a total of 51 data points obtained for use in trajectory fits.
Of those, 16 were for the outer loop, 18 for the cavity, and 17 for the core
feature.
The event times were from 19:34UT until 21:52UT .
The event was visible in MK3 and continued past the LASCO C3 field of view.
Central Position Angle: ~307 - Loop (in degrees) ~305 - Cavity ~303 - CoreThe following data is obtained from performing a second order, least squares fit of the trajectory data points (Hundhausen, et al, 1994) :
Width (degrees): ~45 - Loop (MK3) ~23 - Cavity (MK3)
Start Times (UT): 19:23:31 - Loop 19:30:30 - Cavity 19:34:49 - Core Start Heights (Solar Radii): 1.0 - Loop 1.0 - Cavity 1.0 - Core Final Speeds (km/s): 762.5 - Loop 656.8 - Cavity 579.6 - Core Accelerations (km/s^2): 0.05 - Loop 0.04 - Cavity 0.008 - 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.
| First Order | Second Order |
|---|---|
| (Loop, Cavity, & Core) | (Loop, Cavity & Core) |
|
|
| MK3, C2 and C3 | MK3, C2 and C3 |
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.
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