HINODE Daily Events on 2008/08/19 (Tue)

Station	Pass No. 20080819-	Contact time (UT)		Max. Elev. (deg)	Events
Station	Pass No. 20080819-	AOS	LOS	Max. Elev. (deg)	Events
KRN1	6010	07:08:14	07:21:43	39.2	OP/OG upload XRT: TI-CMD EIS: TI-CMD SOT: TI-CMD
USC34	0200	08:26:27	08:39:28	53.7	OP/OG upload, XRT:TI-CMD, SOT:TI-CMD, EIS:TI-CMD (backup) AOCS: Upload pointing table AOCS: Upload orbital element EIS: Table upload XRT: Table Upload DR playback (by OP)
USC34	0300	10:05:33	10:15:06	10.7	DR playback (by OP) SOT: Table Upload
USC20	0400	20:28:48	20:41:08	19.9	DR playback (by OP)
USC20	0500	22:06:24	22:18:48	30.2	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 [%]	70	15	15
DR allocation [Mbits]	-	-	-
DR TLMLMT [Mbits]	-	-	-

daily note

[Maintenance Note (Morita), for CO/CP/RT Tohban]
The common quick look system will be maintenanced at 10:00-12:00 (JST) on Tuesday the 19th of August.
Please report if you have any trouble.

EIS:
Coronal/transition-region Doppler and photospheric transverse magnetic features associated with cancellation events
- QS near the disk centre, if possible, include an XBP in FOV for alignment
- observation structure similar to the Muglach programme
- run studies in the order: three times (a) - n times (b) -three times (a)
- SOT support:
FG/NFI: NaI/IV 2-wavelength filter (mandatory)
1st priority on the high cadense (at least < 60sec).
2nd priority on the longer coverage (>2-3hrs continuous coverage;
Interuptions by SAAs and S/C nights are OK.)
3rd priority on the FOV (at least, larger than 100arcsec^2)
SP: fast mapping, FOV: same as FG/NFI (mandatory)
FG/BFI: CaII/G-band (lowest priority, can be omitted)
- XRT support:
FOV: cover the same FOV as SOT
Filters: low-temperature filter-pair; Cadence: <5min.

QS Brightenings ( plan for the next day )
- EIS to point at quiet Sun region near disk centre
- request SOT and XRT to observe EIS FoV: 20"X144"

Evolution of X-ray bright point
- point to a quiet region with an X-ray bright point near disk centre
- run for 3 hours or longer; stop during eclipses
- SOT: support with magnetograms (3 min cadence) and Ca II H filtergrams to
track evolution of magnetic fields in the photosphere

XRT:
- Support EIS.

SOT:
- Support EIS.

	CHIEF TOHBAN	SUB TOHBAN	CP	SOT CO	XRT CO	EIS CO
EVENING	Arikawa		Sterling	Kubo	Kano	Akita ( K.Watanabe)
MORNING