Weekly Status Report of the Yohkoh Soft X-Ray Telescope

Updated 24-Oct-97 07:30 UT

Instrument Status

The Soft X-ray Telescope remains in fine working order. The CCD bakeout planned for this week was postponed due to unfavorable scheduling of nighttime. The spacecraft pointing was adjusted to place the Sun's image closer to the center of the SXT images.

A more detailed report of this week's activities is available here.

Observation of the Week

On 23-oct-97, SXT observed the formation of a CME. Flaring loops associated with the event showed motion, and we saw strong coronal dimming in the volume surrounding the brightenings. The flaring loops are shown in the sequence of images below (four-panel box); the growth of the X-ray arcade can be traced during the interval 12:07 to 18:49 UT.

The coronal dimming is evident in the following difference image, which shows the formation of "transient coronal holes" to the northwest and southeast of the bright arcade. The contour shows the zero level in the difference, separating dark (the transient coronal holes) and bright (the arcade).

The coronal dimming can be seen more clearly by measuring the brightness of selected regions and making light curves. An example is shown in the following two images: On the right is an image of the arcade structure, with boxes showing the selected regions of interest. On the left is a graph showing the (normalized) light curves for those two selected regions. The solid line in the graph traces the brightness of the large arcade; the dotted line traces the brightness of the dimming region to the south.

D. McKenzie, H. Hudson 24-Oct-97 (email 'lastname'@isass0.solar.isas.ac.jp)