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

	Date:		20 December 2007
	-----

 	Last revision:	27 December 2007 (Wu)
	--------------

	File Name: 	2007.12.24.a.log
	----------

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

	UVCS Activity:	OVI Detector Diagnostic for December 24 2007
	--------------	South Coronal Hole LYA Observation for 
			24 December 2007
			South Coronal Hole OVI Observation for 
			24 - 25 December 2007

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

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

	Command file:	07.12.21.14:31:55.cmd.log

	Activity:
	---------

	1) OVI Detector Diagnostic

	Sequence: OVI_164_chk.tcl

	SCI_SPEC: 

	OBS_PROG: Spatial Resolution

	SCI_OBJ:  

	OBJ:      Coronal Hole

	CMP_NAME: 

	CMP_NUM:  

	Duration: start: 2007.12.24.15:02
                    end: 2007.12.24.16:03

	ONUMs =	23916 (12 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll: 180 Degrees

		- Roll:  180 Degrees (18762) 

		- Mirror/Occulter:  1.75 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_chk_1xfull in slot 6

	Fits Files:

q07.12.24.14:52:28.ovi.dat

	2) South Coronal Hole Observations

	Sequence: 08.01_hole.tcl, n = 1, m = 0, p = 0, r = 1, e = 0

	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: 2007.12.24.16:06
		    end: 2007.12.24.19:08

	ONUMs = 23917 (88 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	172.09 Degrees (17322)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_sp2_164 in slot 4

	Fits Files:

q07.12.24.16:05:58.ovi.dat

	3) South Coronal Hole Observations

	Sequence: 08.01_hole.tcl, n = 8, m = 1, p = 0, r = 1, e = 0

	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: 2007.12.24.19:10
		    end: 2007.12.25.18:10

	ONUMs = 23918 (320 exps)   
		23919 (347 exps)

	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  180 Degrees

		- Roll:	172.09 Degrees (17322)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

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

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask:   OVI_EclipSyn_215 in slot 2

	Fits Files:

q07.12.24.19:09:37.ovi.dat
q07.12.25.06:10:57.ovi.dat

GAP between 12/25/07|10:14:23(13027) and 12/25/07|10:15:25(13127)