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

	Date:		01 October 2007
	-----

 	Last revision:	05 October 2007 (MU)
	--------------

	File Name: 	2007.10.02.a.log
	----------

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

	UVCS Activity:  Flush IQ/BQ
	--------------	Reload and Continue Equatorial Coronal Hole OVI 
                        Observation for 01 - 02 October 2007
			Load Equatorial Coronal Hole OVI Observation for 
			02 October 2007
		 	Load North Coronal Hole OVI Observation for 
			02 - 03 October 2007
			Load North Coronal Hole OVI Observation for 
			03 - 04 October 2007
			Load OVI Detector Diagnostic for 04 October 2007
			Load North Coronal Hole LYA Observation for 
			04 October 2007
			Load North Coronal Hole OVI Observation for 
			04 - 05 October 2007
                        Load North Coronal Hole OVI Observation for 
                        05 - 06 October 2007

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

	EOF Staff:      S. Cranmer: Lead Scientist
	---------- 	M. Uzzo: Planner
			Y.-K. Ko: Commander

	Command file:	07.10.01.13:05:36.cmd.log
                        07.10.02.15:18:12.cmd.log

	Activity:
	---------

	1) Equatorial Polar Coronal Hole OVI Observations

	Sequence: 06.08_hole.tcl, n = 1, m = 0, p = 1, r = 0, e = 0

	SCI_SPEC: Characterization of an equatorial coronal hole.
		  Goal is to measure the properties of an equatorial
		  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 polar coronal holes.

		  Roll positions are VL-corrected for PA=245 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: 2007.10.02.20:17
		    end: 2007.10.02.23:23

	ONUMs = 23725 (90 exps)   
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	237.09 Degrees (61944)

		- 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:

q07.10.02.20:17:36.ovi.dat


	2) North Polar Coronal Hole OVI Observations

	Sequence: 06.08_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=0 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: 2007.10.02.23:48
		    end: 2007.10.03.22:49

	ONUMs = 23726 (320 exps)   
		23727 (344 exps)
		
	Instrument configuration:

		- Pointing:  Sun center

                - Spacecraft Roll:  0 Degrees

		- Roll:	353.267 Degrees (17536)

		- Mirror/Occulter:  2.0 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:

q07.10.02.23:48:32.ovi.dat
q07.10.03.10:49:52.ovi.dat

GAP between 10/03/07|13:25:38(  921) and 10/03/07|13:30:38( 1400)
GAP between 10/03/07|14:44:19( 8482) and 10/03/07|14:45:21( 8583)