UVCS MISSION LOG 
				----------------

	Date:		30 December 2003
	-----

 	Last revision:	06 January 2004 (Ko)
	--------------

	File Name: 	2003.12.31.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	North Coronal Hole Observation for 
	--------------	31 December 2003 - 01 January 2004
			Load Mini-Synoptic for 01 January 2004 using Batch
			Queue Time Tagged Commands via NRT

	SOHO Activity:	
        --------------  

	EOF Staff:	J. Kohl: Lead Scientist
	----------	M. Uzzo / R. Wu: Commander
			M. Uzzo: Planner
			Y.-K. Ko

	Command file:	03.12.30.18:53:08.cmd.log

	Activity:
	---------

	1) Observation of the North Coronal Hole

	Sequence: 03.12_hole5short2.tcl, n53min=6

	SCI_SPEC: Characterization of a polar coronal hole.
                  Goal is to measure the properties of a polar
                  coronal hole. In particular we are interested in the 
                  coronal conditions (intensities and line widths for 
                  HI Ly-alpha and OVI 1032/1037) as a function of height 
                  and latitude. We will compare these properties with 
                  the ones found in non-polar coronal holes.

		  Roll positions are VL-corrected for PA=335 degrees.

	OBS_PROG: Primary: Sensitivity
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Proton and Ion Temperatures

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2003.12.31.18:20
                    end: 2004.01.01.00:19

	ONUMs =	20703 (23 exps)
		20704 (120 exps)
		20705 (15 exps)
		
	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 328.27, 327.09, 328.277 degrees (45775, 45560, 45775)
 
		- Mirror/Occulter:  2.0, 1.7, 2.0 Ro
                                    1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:    50 um 

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 170300

		- LYA mask:   LYA_93_1sec   in slot 2
		- OVI mask:   OVI_170300MPM in slot 5

	Fits Files:

q03.12.31.18:19:31.lya.dat
q03.12.31.18:19:31.ovi.dat
q03.12.31.18:19:31.vld.dat

GAP between 12/31/03|18:30:25( 2678) and 12/31/03|18:37:12( 3330)

q03.12.31.19:19:48.lya.dat
q03.12.31.19:19:48.ovi.dat
q03.12.31.19:19:48.vld.dat
q03.12.31.23:46:21.lya.dat
q03.12.31.23:46:21.ovi.dat
q03.12.31.23:46:21.vld.dat

	2) Mini-Synoptic Sequence Load and Start

	Sequence: SynopticA:Mini

	SCI_SPEC: Synoptic studies.  LYA HV off / OVI voltage at 215,
		  LYA grating position now at 128000 "permanently".

		  NB: DSN coverage pre-empted by VIRGO record time.
		  Any missing data should be recoverable after Keyhole.

		  NB: 06 January 2004, data have been recovered.

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2004.01.01.08:12
		    end: 2004.01.01.11:39

	ONUMs = 44190 (9 exps)
		44191 (9 exps)
		44192 (9 exps)
		44193 (9 exps)
		44194 (9 exps)
		44195 (9 exps)
		44196 (9 exps)
		44197 (9 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  180 Degrees

		- Roll: E, SE, S, SW, W, NW, N, NE

		- Mirror/Occulter: 1.6, 1.75 Ro
 				   1.5 mm overocculting (1.6 Ro)
				   2.0 mm overocculting (1.75 Ro)

		- LYA Slits:   50 um
		- OVI Slits:  150 um

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 184200

		- LYA mask:   LYA_93_1sec in slot 2
		- OVI mask:   OVI_Syn_184 in slot 2

	Fits Files:

GAP between 01/01/04|08:10:20(15921) and 01/01/04|08:13:03(16182)

z04.01.01.08:11:18.lya.dat
z04.01.01.08:11:18.ovi.dat
z04.01.01.08:11:18.vld.dat
z04.01.01.08:37:49.lya.dat
z04.01.01.08:37:49.ovi.dat
z04.01.01.08:37:49.vld.dat
z04.01.01.09:04:18.lya.dat
z04.01.01.09:04:18.ovi.dat
z04.01.01.09:04:18.vld.dat
z04.01.01.09:30:47.lya.dat
z04.01.01.09:30:47.ovi.dat
z04.01.01.09:30:47.vld.dat
z04.01.01.09:57:30.lya.dat
z04.01.01.09:57:30.ovi.dat
z04.01.01.09:57:30.vld.dat
z04.01.01.10:23:59.lya.dat
z04.01.01.10:23:59.ovi.dat
z04.01.01.10:23:59.vld.dat
z04.01.01.10:50:28.lya.dat
z04.01.01.10:50:28.ovi.dat
z04.01.01.10:50:28.vld.dat
z04.01.01.11:16:55.lya.dat
z04.01.01.11:16:55.ovi.dat
z04.01.01.11:16:55.vld.dat