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

	Date:		30 October 2007
	-----

 	Last revision:	20 November 2007 (Wu)
	--------------

	File Name:	2007.10.31.a.log
 	----------

	Compiled by:	M. Uzzo, R. Wu, Y.-K. Ko
	------------

	UVCS Activity:	SOHO / Hinode Polar Plumes LYA Campaign for 
	--------------	31 October 2007
			SOHO / Hinode Polar Plumes OVI Campaign for 
			31 October - 01 November 2007
			SOHO / Hinode Polar Plumes LYA Campaign for 
			01 November 2007

	SOHO Activity:	Received via email Thursday, 01 November 2007,  
	--------------	02:00:42 GMT: OBT DISTRIBUTED TO UVCS BY FOT

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

	Command file:	07.10.30.12:44:09.cmd.log

	Activity:
	---------

	1) SOHO/Hinode Polar Plumes Campaign, JOP197

	Sequence: 07.10_Plume_lyared.tcl

        SCI_SPEC: To characterize the physical parameters (densities, temperatures,
                  abundance, flows) of coronal hole plumes with coordinated multi-spacecraft
                  observations, and relate changes in the photospheric magnetic fields with
                  changes in the observed plasma properties in order to understand the
                  physical processes that lead to the formation of these stable structures.

        OBS_PROG: Temporal Coverage
                  Spatial Coverage

        SCI_OBJ:  Coronal Structure...Fine Structure
                  Coronal Dynamics...Outflow Velocities
                  Roll angle is such that row 290 is at the target angle of PA=0 degree

        OBJ:      Polar Plume

	CMP_NAME: Multi-wavelength observations of coronal hole plumes at 
		  solar minimum, JOP197 

	CMP_NUM:  7243

	Duration: start: 2007.10.31.17:04
                    end: 2007.10.31.19:04

	ONUMs =	23793 (58 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll: 20.0 Degrees (22400)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   200 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask: OVI_sp2_164 in slot 4

	Fits Files:

q07.10.31.17:04:15.ovi.dat

	2) SOHO/Hinode Polar Plumes Campaign, JOP197

	Sequence: 07.10_Plume_ovi.tcl, n3h = 8, n50m = 2, n21m = 1

	SCI_SPEC: To characterize the physical parameters (densities, 
		  temperatures, abundance, flows) of coronal hole plumes 
		  with coordinated multi-spacecraft observations, and relate 
		  changes in the photospheric magnetic fields with changes 
		  in the observed plasma properties in order to understand 
		  the physical processes that lead to the formation of these 
		  stable  structures.

                  Roll angle is such that row 290 is at the target angle of 
                  PA = 0 degrees

	OBS_PROG: Primary: Temporal Coverage
                  Sub Obj: Spatial Coverage

	SCI_OBJ:  Primary: Coronal Structure...Fine Structure
                  Sub Obj: Coronal Dynamics...Outflow Velocities

        OBJ:      Polar Plume

	CMP_NAME: Multi-wavelength observations of coronal hole plumes at 
		  solar minimum, JOP197 

	CMP_NUM:  7243

	Duration: start: 2007.10.31.19:05
                    end: 2007.11.01.19:08

	ONUMs =	23794 (240 exps)
		23795 (240 exps)
		23796 (218 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll: 20.0 Degrees (22400)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   200 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 217000

		- OVI MCP Voltage: 200 

		- OVI mask: OVI_Plume_217 in slot 1

	Fits Files:

q07.10.31.19:05:23.ovi.dat
q07.11.01.03:21:23.ovi.dat
q07.11.01.11:37:23.ovi.dat

	3) SOHO/Hinode Polar Plumes Campaign, JOP197

	Sequence: 07.10_Plume_lyared.tcl

        SCI_SPEC: To characterize the physical parameters (densities, temperatures,
                  abundance, flows) of coronal hole plumes with coordinated multi-spacecraft
                  observations, and relate changes in the photospheric magnetic fields with
                  changes in the observed plasma properties in order to understand the
                  physical processes that lead to the formation of these stable structures.

        OBS_PROG: Temporal Coverage
                  Spatial Coverage

        SCI_OBJ:  Coronal Structure...Fine Structure
                  Coronal Dynamics...Outflow Velocities
                  Roll angle is such that row 290 is at the target angle of PA=0 degree

        OBJ:      Polar Plume

	CMP_NAME: Multi-wavelength observations of coronal hole plumes at 
		  solar minimum, JOP197 

	CMP_NUM:  7243

	Duration: start: 2007.11.01.19:09
                    end: 2007.11.01.21:09

	ONUMs =	23797 (58 exps) 

	Instrument configuration:

		- Pointing:  Sun center

		- Spacecraft Roll:  0 Degrees

		- Roll: 20.0 Degrees (22400)

		- Mirror/Occulter:  1.7 Ro
				    1.5 mm overocculting

		- LYA Slit:   100 um
		- OVI Slit:   200 um 

		- LYA GRTPOS: 100000
		- OVI GRTPOS: 164600

		- OVI MCP Voltage: 200 

		- OVI mask: OVI_sp2_164 in slot 4

	Fits Files:

q07.11.01.19:09:11.ovi.dat