HINODE Daily Events on 2023/07/04 (Tue)

Station	Pass No. 20230704-	Contact time (UT)		Max. Elev. (deg)	Events
Station	Pass No. 20230704-	AOS	LOS	Max. Elev. (deg)	Events
MSP1	8000	07:20:54	07:34:11	42.6	OP/OG upload XRT: TI-CMD EIS: TI-CMD
USC20	0100	08:27:42	08:39:40	20.2	OP/OG upload, XRT:TI-CMD, EIS:TI-CMD (backup) AOCS: Upload pointing table AOCS: Upload orbital element EIS: Table Upload DR playback (by OP)
MSP1	8010	08:58:56	09:09:43	12.7	XRT: Table Upload
USC20	0200	10:04:17	10:16:24	28.7	Backup for Table Uploads DR playback (by OP)
USC34	0400	22:04:25	22:17:54	85.1	DR playback (by OP)

Flare list(LM) : http://www.lmsal.com/solarsoft/last_events/

DR information

OP main: 2023/07/04 10:44:00 - 2023/07/11 11:31:00 (UT)

Remaining amount
(prediction)

2818 Mbits @ OP_START ( 2023/07/04 10:44:00 )

DR usage: The DR would become empty on Jul 5 at 6 UT if all telescopes took no images until that time.

	SOT	XRT	EIS
DR allocation [%]	54	23	23
DR allocation [Mbits]	12271	5226	5226
DR TLMLMT [Mbits]	2102 @OP_START -> 15604	6586	6586

daily note

Co-alignment program run:
Please run co-alignment program during the period for the three instruments.
- If the solar condition is not permitted, please delay to the next timeline.
- The sequence should start exactly 15 minutes after the pointing change to stabilize the satellite pointing drift.
- 2 hours for N-limb at *** 930*** arcsec and 2 hours for E limb at *** -970*** arcsec.
- Not necessary to be during SAA-free time.
- For XRT, take G-band data every 5 minutes instead of 8 minutes. This is just for the N limb run. 8 minutes cadence is still OK for the E limb run.
- For XRT, please take data even during SAA and twilight periods.
- For SOT, please use CTM HYSTERISIS (not CT RUN) at the start of each SP program
- For EIS, please run Imada's new co-alignment program

SOT:
- HOP 081 (2023/07/04,2023/07/06)
- HOP 393 (2023/07/08)
- HOP 467
- AR obs.

XRT:
- HOP 081 (2023/07/04,2023/07/06)
- HOP 349
- HOP 393 (2023/07/08)
- HOP 448
- HOP 467

EIS:
HOP 081 (2023/07/04,2023/07/06)
HOP 393 - Equatorial Transition
HOP 467 - STEREO/SECCHI High Telemetry Campaign
Evolution of abundances in AR core loops and microflares
Coronal Magnetic Field Measurements in Flares (run on any active region)
Quiet Sun run of EIS Spectral Atlas Synoptic Programme

	CHIEF TOHBAN	SUB TOHBAN	CP	SOT CO	XRT CO	EIS CO
EVENING	Kotanagi		Arai	Yoshitake	Arai	Hansteen
MORNING