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

	Date:		08 February 2005
	-----

 	Last revision:	09 February 2005 (Wu)
	--------------

	File Name: 	2005.02.08.a.log
	----------

	Compiled by:   	Y.-K. Ko
	------------

	UVCS Activity:  Load and Start South Polar Coronal Hole OVI Observation for
	--------------  08 - 09 February 2005
                        Load OVI Synoptic for 09 February 2005
			Load South Polar Coronal Hole LyA Observation for 
			09 February 2005
			Load South Polar Coronal Hole OVI Observation for 
			09 - 10 February 2005
			Load South Polar Coronal Hole OVI Observation for 
			10 February 2005
			Load Mini-Synoptic for 10 February 2005

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

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

	Command file:	05.02.08.15:02:12.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observation 

	Sequence: 05.02_hole1OVI.tcl

	SCI_SPEC: Characterization of the 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 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: 2005.02.08.18:39
                    end: 2005.02.09.04:05

	ONUMs =	22089 (105 exps)  
		22090 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 177.09, 178.27, 179.38 degrees (18233, 18447, 18649)

		- 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: 230000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_MPM_232 in slot 5

	Fits Files:

q05.02.08.18:27:19.ovi.dat
q05.02.08.22:17:04.ovi.dat

	2) 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: 2005.02.09.04:14
		    end: 2005.02.09.18:28

	ONUMs = 47240 (49 exps)
		47241 (49 exps) 
		47242 (47 exps) 
		47243 (47 exps) 
		47244 (49 exps) 
		47245 (49 exps) 
		47246 (46 exps) 
		47247 (49 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:	E: os, SE: os, S: oc, SW: os,
			W: os, NW: os, N: oc, NE: 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:   50 um
		- OVI Slits:  150 um (LyA Synoptic)
			      200 um (OVI, and Mini Synoptic)

		- LYA GRTPOS: 128000
		- OVI GRTPOS: 187260 (LyA Synoptic)
			      229000 (OVI, and Mini Synoptic)

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_188 in slot 6 (LyA Synoptic)
			      OVI_Syn_230 in slot 1 (OVI, and Mini Synoptic)

	Fits Files:

z05.02.09.04:14:18.ovi.dat
z05.02.09.06:02:58.ovi.dat
z05.02.09.07:51:38.ovi.dat
z05.02.09.09:35:05.ovi.dat

GAP between 02/09/05|09:42:01(12251) and 02/09/05|09:45:12(12551)

z05.02.09.11:23:45.ovi.dat
z05.02.09.13:12:25.ovi.dat
z05.02.09.15:01:05.ovi.dat

GAP between 02/09/05|16:42:24( 3483) and 02/09/05|16:45:22( 3765)

z05.02.09.16:44:32.ovi.dat