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

	Date:		11 January 2006
	-----

 	Last revision:	17 February 2006 (Wu)
	--------------

	File Name:	2006.01.11.a.log
	----------

	Compiled by:	R. Wu
	------------

	UVCS Activity:	Load and Start South Polar Coronal Hole LyA Observation
        --------------  for 11 January 2006
        		Load South Polar Coronal Hole OVI Observation for
        		11 - 12 January 2006
        		Load OVI Synoptic for 12 January 2006

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

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

	Command file:	06.01.11.17:13:00.cmd.log

	Activity:
	---------

	1) South Polar Coronal Hole Observation 

	Sequence: 06.01_hole2LyA.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=180 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: 2006.01.11.1
                    end: 2006.01.11.2

	ONUMs =	22106 (57 exps)  

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 352.09, 354.38 degrees (17323, 17739)

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

		- LYA Slit:   100 um
		- OVI Slit:    50, 75 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp1_164 in slot 4

	Fits Files:

q06.01.11.19:10:02.ovi.dat

	2) South Polar Coronal Hole Observation 

	Sequence: 06.01_hole2OVI.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=180 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: 2006.01.11.21:20
                    end: 2006.01.12.07:21

	ONUMs =	22107 (74 exps)  
		22108 (216 exps)

	Instrument configuration:

		- Pointing:  Sun Center

		- Spacecraft Roll: 180 Degrees

		- Roll: 352.09, 354.38 degrees (17323, 17739)

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

		- LYA Slit:   100 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:

q06.01.11.21:19:47.ovi.dat
q06.01.11.23:53:15.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: 2006.01.12.07:30
		    end: 2006.01.12.21:44

	ONUMs = 49340 (48 exps)
		49341 (48 exps) 
		49342 (47 exps)
		49343 (49 exps)
		49344 (49 exps)
		49345 (49 exps)
		49346 (47 exps)
		49347 (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 Slit:   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:

z06.01.12.07:29:50.ovi.dat
z06.01.12.09:18:30.ovi.dat
z06.01.12.11:07:10.ovi.dat
z06.01.12.12:50:38.ovi.dat
z06.01.12.14:39:18.ovi.dat
z06.01.12.16:27:58.ovi.dat
z06.01.12.18:16:38.ovi.dat
z06.01.12.20:00:05.ovi.dat