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

	Date:		24 November 2004
	-----

 	Last revision:	06 December 2004 (Wu)
	--------------

	File Name:	2004.11.27.a.log
	----------

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

	UVCS Activity:	South Coronal Hole LyA Observation for 27 November 2004
	--------------	West Scan of Mini-Synoptic for 27 November 2004
			Ulysses-SOHO Quadrature for 27-28 November 2004				

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

	EOF Staff:      S. Cranmer / G. Poletto: Lead Scientist
	----------	M. Uzzo: Commander, Planner
			R. Wu

	Command file:	04.11.24.12:38:13.cmd.log

	Activity:
	---------

	1) South Coronal Hole Observation 

	Sequence: 04.11_hole1LyA.tcl

	SCI_SPEC: Characterization of a south 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=185 degree.

	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: 2004.11.27.13:41
                    end: 2004.11.27.18:15

	ONUMs =	21840 (132 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 177.09, 178.27, 179.38 degrees (51021, 51236, 51438)
 
		- Mirror/Occulter:  1.7, 2.0, 2.4 Ro
			            1.5 mm overocculting

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

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 187470

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_188 in slot 6

	Fits Files:

q04.11.27.13:33:19.ovi.dat

	2) West Scan Only of Mini-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: 2004.11.27.18:43
		    end: 2004.11.27.19:02

	ONUMs = 46849 (9 exps)

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll:	W: ms

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

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 177596 (LyA Synoptic)
			      229000 (OVI, and Mini Synoptic)

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_Syn_178 in slot 2 (LyA Synoptic)
			      OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic)

	Fits Files:

z04.11.27.18:42:08.ovi.dat

	3) Ulysses-SOHO Quadrature 

	Sequence: 04.11_ulysses.tcl

	SCI_SPEC: Physical parameters in the range of 1 to 2 Ro from 
		  coordinated SUMER-UVCS observations and comparison 
		  with in situ data collected at the time of 
		  SOHO-Sun-Ulysses quadrature.

	OBS_PROG: Primary: Spectral Coverage
		  Sub Obj: Spatial Coverage

	SCI_OBJ:  Plasma Properties...Abundances and Electron Temperatures

	OBJ:      Streamer Boundary

	CMP_NAME: Ulysses Quadrature, UVCS; SUMER; Ulysses (S/C)

	CMP_NUM:  7101

	Duration: start: 2004.11.27.19:37
                    end: 2004.11.28.09:33

	ONUMs =	21841 (240 exps) 
		21842 (80 exps)
		21843 (8 exps)
		21844 (75 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll:  0 Degrees

		- Roll: 252 degrees (64658)
 
		- Mirror/Occulter:  1.6 Ro
			            1.5 mm overocculting

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

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 232100, 187470, 86600

		- OVI MCP Voltage: 200 

		- OVI mask:  OVI_sp2_188 in slot 5
			     OVI_303_2x6 in slot 4

	Fits Files:

q04.11.27.19:35:59.ovi.dat
q04.11.28.03:53:09.ovi.dat
q04.11.28.06:38:29.ovi.dat
q04.11.28.06:56:16.ovi.dat