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

	Date:		19 October 2005
	-----

 	Last revision:	17 November 2005 (Wu)
	--------------

	File Name:	2005.10.23.a.log
	----------

	Compiled by:	M. Uzzo
	------------

	UVCS Activity:	Polar Coronal Hole OVI Observation for 
	--------------	23 - 24 October 2005
			OVI Synoptic for 24 October 2005

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

	EOF Staff:      M. P. Miralles: Lead Scientist
	---------- 	M. Uzzo: Commander, Planner
			Y.-K. Ko
			R. Wu

	Command file:	05.10.21.14:12:37.cmd.log

	Activity:
	---------

	1) Polar Coronal Hole Observation 

	Sequence: 05.09_hole1OVI.tcl

	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=8 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: 2005.10.23.23:48
                    end: 2005.10.24.09:14

	ONUMs =	21865 (98 exps)  
		21866 (164 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 0.093, 1.267, 2.381 degrees (18779, 18993, 19195)

		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
			            1.5 mm overocculting (1.7, 2.0 Ro)
			            2.0 mm overocculting (2.4 Ro)

		- LYA Slit:    50 um
		- OVI Slit:    50, 75 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q05.10.23.23:38:57.ovi.dat

GAP between 10/24/05|00:21:50( 9760) and 10/24/05|00:22:52( 9860)
GAP between 10/24/05|00:33:50(10914) and 10/24/05|00:49:02(12370)

q05.10.24.03:25:51.ovi.dat

GAP between 10/24/05|05:15:17( 5185) and 10/24/05|05:24:45( 6088)

	2) OVI Synoptic Sequence Load and Start

	Sequence: SynopticD:Start

	SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage 
		  at 200.

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2005.10.24.09:24
		    end: 2005.10.24.23:38

	ONUMs = 48900 (49 exps)
		48901 (49 exps) 
		48902 (47 exps)
		48903 (49 exps)
		48904 (49 exps)
		48905 (49 exps)
		48906 (47 exps)
		48907 (49 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 0 Degrees

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

		- Mirror/Occulter:

			ls:	3.00, 2.50, 2.10, 1.90, 1.75, 1.60 Ro
			lc:	2.10, 1.90, 1.75, 1.60 Ro
			os:	3.00, 2.10, 1.90, 1.75, 1.60 Ro
			oc:	1.90, 1.75, 1.60 Ro
			ms:	2.10, 1.75, 1.60 Ro
			mc:	1.90, 1.75, 1.60 Ro

			1.5 mm overocculting (1.60 Ro)
			2.0 mm overocculting (1.75, 1.90, 2.10, 2.50, 3.00 Ro)

		- LYA Slits:  100 um
		- OVI Slits:  150 um (LyA Synoptic)
			      200 um (OVI, and Mini Synoptic)

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 187260 (LyA Synoptic)
			      229000 (OVI, and Mini Synoptic)

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Syn_188 in slot 2 (LyA Synoptic)
			      OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic)

	Fits Files:

z05.10.24.09:23:26.ovi.dat
z05.10.24.11:12:06.ovi.dat
z05.10.24.13:00:46.ovi.dat
z05.10.24.14:44:13.ovi.dat
z05.10.24.16:32:53.ovi.dat
z05.10.24.18:21:33.ovi.dat
z05.10.24.20:10:13.ovi.dat
z05.10.24.21:53:41.ovi.dat