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

	Date:		09 May 2005
	-----

 	Last revision:	07 July 2005 (MU)
	--------------

	File Name:	2005.05.09.a.log
	----------

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

	UVCS Activity:	Load and Start North Polar Coronal Hole LyA Observation
        --------------  for 09 - 10 May 2005
			Load North Polar Coronal Hole OVI Observation
        	        for 10 May 2005
			Load Mini-Synoptic for 10 May 2005

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

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

	Command file:	05.05.09.15:56:31.cmd.log

	Activity:
	---------

	1) North Polar Coronal Hole Observation 

	Sequence: 05.02_hole1LyA.tcl

	SCI_SPEC: Characterization of the North 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=351 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: 2005.05.09.23:29
                    end: 2005.05.10.04:03

	ONUMs =	22339 (132 exps) 

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 0 Degrees

		- Roll: 343.09, 344.27, 345.38 degrees (15684, 15898, 16101)

		- 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: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_164 in slot 4

	Fits Files:

q05.05.09.23:18:28.ovi.dat

	2) North Polar Coronal Hole Observation 

	Sequence: 05.02_hole1OVI.tcl

	SCI_SPEC: Characterization of the North 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=351 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: 2005.05.10.04:05
                    end: 2005.05.10.13:30

	ONUMs =	22340 (105 exps)  
		22341 (168 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 0 Degrees

		- Roll: 343.09, 344.27, 345.38 degrees (15684, 15898, 16101)

		- 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:

q05.05.10.04:03:44.ovi.dat
q05.05.10.07:42:41.ovi.dat

	3) 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: 2005.05.10.13:39
		    end: 2005.05.10.18:41

	ONUMs = 47950 (9 exps)
		47951 (9 exps) 
		47952 (35 exps)
		47953 (9 exps)
		47954 (9 exps)
		47955 (9 exps)
		47956 (35 exps)
		47957 (9 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll: 0 Degrees

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

z05.05.10.13:38:37.ovi.dat
z05.05.10.14:03:33.ovi.dat
z05.05.10.14:28:29.ovi.dat
z05.05.10.15:47:08.ovi.dat
z05.05.10.16:12:04.ovi.dat
z05.05.10.16:37:00.ovi.dat
z05.05.10.17:01:56.ovi.dat
z05.05.10.18:20:35.ovi.dat