CHIEF OBSERVER'S REPORT for Week 27
28-Jun-99 to 4-Jul-99
July 5, 1999
B. Handy, H. Hudson

GENERAL

Activity was very high, with numerous M flares but no X flares. Maybe there is something to the suggestion that the biggest flares happen mainly in the rising and decaying phases of a solar maximum?

SXT TECHNICAL

We've finished a whole cycle of terminator image acquisition, completing the database that began April 18. Accordingly, on July 2, we re-defined the normal pointing of Yohkoh to move the solar image 40" to the E (S/C to the W) and we hope that this will reduce the occurrence of dark-current artifacts at the NW limb.

We will plan to do a CCD bakeout following the computer outage next week.

SXT SCIENCE

For Web material see

Current Week: http://www.solar.isas.ac.jp/sxt_co/SXTweekly.html
Current Week: http://www.solar.isas.ac.jp/sxt_co/990701.html
Index: http://www.solar.isas.ac.jp/sxt_co/index.html

CAMPAIGNS

For more information on campaigns, see:

http://sec.noaa.gov/solcoord/solcoord.html

For SXT plans, finger campaign@isass0.solar.isas.ac.jp.

PERSONNEL

Piet Martens departed on Friday.

SEMINARS

Brian Handy gave a talk July 1 on C IV observations from TRACE. We failed to succeed in projecting his movies, but he has pure C IV time-series imagery - quite interesting.

SXT TABLE PLAN, WEEK 28
(4-Jul-99 to 10-Jul)

We are not aware of any special campaign activities this week, but will as usual try to coordinate with SOHO and TRACE if possible.


JST Day         UT Start Time      Pass   Table ID

Monday           5-JUL-99 05:42    2      950705 P2 ARS1 STANDARD 
Tuesday          6-JUL-99 09:21    3      950706 P3 ARS1 DARK 
Wednesday        7-JUL-99 09:36    3      950707 P3 ARS1 DIFFUSER 
Thursday         8-JUL-99 06:25    2      960708 P2 ARS1 STANDARD
Friday           9-JUL-99 06:40    3      960709 P3 ARS1 STANDARD 
Saturday        10-JUL-99 06:55    3      960710 P3 ARS1 STANDARD 

This plan is subject to change.

Continuing requests:

KSC & SSOC Tohbans: If any KSC passes are likely to be cancelled (for example due to a typhoon) or an SXT table cannot be uploaded for some reason, please telephone and e-mail the Chief Observer immediately. (sxt_co@isass0.solar.isas.ac.jp, copy to sxt_st@flare2.solar.isas.ac.jp).

SSOC Tohban: On the weekly visible diagram, please mark the official five passes first and then cross out those passes that will be given to other satellites. That way we can keep the numbering straight in the Yohkoh software system.

SSOC Tohban: SXT operations do not currently include terminator off- pointing. It is unnecessary this week to ask the SXT Chief Observer for terminator off-pointing information.

KSC Tohbans: In general flare mode supersedes table upload, i.e. if a flare is in progress please do not upload a new table, and contact the chief observer. Normally it is OK to go ahead with the planned table without change on the next pass, if it is available. Chief observers should keep an eye on this.