HINODE Daily Events on 2017/12/12 (Tue)

Station	Pass No. 20171212-	Contact time (UT)		Max. Elev. (deg)	Events
Station	Pass No. 20171212-	AOS	LOS	Max. Elev. (deg)	Events
USC20	0100	07:42:53	07:54:31	17.9	OP/OG upload XRT: TI-CMD EIS: TI-CMD XRT: CCD Bakeout Heater is ON DR playback (by OP)
USC20	0200	09:19:14	09:31:26	32.1	OP/OG upload, XRT:TI-CMD, EIS:TI-CMD (backup) AOCS: Upload pointing table AOCS: Upload orbital element EIS: Table Upload XRT: CCD Bakeout Heater is ON DR playback (by OP)
SNT1	4000	10:08:45	10:22:41	87.6	XRT: Table Upload XRT: CCD Bakeout Heater is ON
USC20	0400	21:19:39	21:33:23	85.0	XRT: CCD Bakeout Heater is ON DR playback (by OP)
USC20	0500	22:59:37	23:06:25	7.0	XRT: CCD Bakeout Heater is ON DR playback (by OP)

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

DR information

Remaining amount
(prediction)

- Mbits @ OP_START ( )

	SOT	XRT	EIS
DR allocation [%]	44	28	28
DR allocation [Mbits]	-	-	-
DR TLMLMT [Mbits]	-	-	-

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

XRT:
- CCD bakeout (2017/12/10-2017/12/13) --> Started 2017/12/10 06:27:00 UT
- AR observations

SOT:
- co-alignment program
- HOP 0335 (Observation-Driven Modelling of Solar Phenomena) on 2017/12/13
- AR on SE limb

EIS:
- HOP 0130 (Multi-temperature Full Disk Slot Scans) on 2017/12/12
- HOP 0335 (Observation-Driven Modelling of Solar Phenomena) on 2017/12/13
- AR observations

	CHIEF TOHBAN	SUB TOHBAN	CP	SOT CO	XRT CO	EIS CO
EVENING	Hosoi		Hosoi	Otsuji	Yoshimura (RCO)	Hansteen (RCO)
MORNING