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

	Date:		03 November 2005
	-----

 	Last revision:	15 November 2005 (Wu)
	--------------

	File Name:	2005.11.03.a.log
	----------

	Compiled by:	M. Uzzo, R. Wu
	------------

	UVCS Activity:	Ramp Down and Turn Off LYA HV and Detector Power
	--------------	Turn On OVI Detector Power
			Conduct OVI Stimulus Pulse Test 
			Load OVI Detector Mask OVI_str_164_225 into OVI slot 6
			Turn On and Ramp Up OVI HV
			Load and Start Polar Coronal Hole OVI Observation for 
			03 - 04 November 2005
			Load OVI Synoptic for 04 November 2005

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

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

	Command file:	05.11.03.17:02:17.cmd.log

	Activity:
	---------

	1) OVI Stimulus Pulse Test

	Sequence: Manual

	SCI_SPEC: To confirm that the OVI detector is functioning nominally,
		  Stimulus Pulse enabled for the exposures with High 
		  Voltage Power Supply powered off.  

	OBS_PROG: 

	SCI_OBJ:  

	OBJ:      

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2005.11.03.17:52
                    end: 2005.11.03.17:56

	ONUMs =	21895 (2 exps)
                
	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 0 Degrees

		- Roll: 120 degrees (40617)
 
		- Mirror/Occulter:  3.5 Ro
			            1.5 mm overocculting

		- LYA Slit:    50 um
		- OVI Slit:   100 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 176000

		- LYA MCP Voltage: 0 
		- OVI MCP Voltage: 0 

		- OVI DETECTOR POWERED ON
		- LYA DETECTOR POWERED OFF

		- OVI mask:   msk_000303_OVI in slot 3

	Fits Files:

q05.11.03.17:50:31.ovi.dat

	2) 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=195 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: 2005.11.03.18:30
                    end: 2005.11.04.03:56

	ONUMs =	21896 (105 exps)  
		21897 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 187.093, 188.267, 189.381 degrees (52842, 53056, 53259)

		- 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:

q05.11.03.18:29:03.ovi.dat
q05.11.03.22:07:53.ovi.dat

	3) OVI Synoptic Sequence Load and Start

	Sequence: SynopticD:Start

	SCI_SPEC: Synoptic studies. VLD & LYA HV & Power off / OVI voltage 
		  at 200, LYA grating position now at 128000 "permanently".

	OBS_PROG: Synoptic

	SCI_OBJ:  Synoptic

	OBJ:      Entire Corona

	CMP_NAME:

	CMP_NUM:

	Duration: start: 2005.11.04.04:01
		    end: 2005.11.04.18:14

	ONUMs = 48930 (49 exps)
		48931 (25 exps) 
		48932 (38 exps)
		48933 (47 exps)
		48934 (49 exps)
		48935 (47 exps)
		48936 (49 exps)
		48937 (49 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 0 Degrees

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

z05.11.04.04:00:09.ovi.dat
z05.11.04.05:48:49.ovi.dat

GAP between 11/04/05|06:42:27(11678) and 11/04/05|07:55:24( 2301)

z05.11.04.07:32:17.ovi.dat
z05.11.04.09:20:57.ovi.dat

GAP between 11/04/05|10:46:44( 2379) and 11/04/05|10:50:42( 2756)
GAP between 11/04/05|10:52:27( 2923) and 11/04/05|10:53:52( 3056)

z05.11.04.11:09:37.ovi.dat
z05.11.04.12:58:17.ovi.dat
z05.11.04.14:41:45.ovi.dat
z05.11.04.16:30:25.ovi.dat