<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2008-02-11T04:38:30Z"
	version="1.11"
	xmlns="http://www.ivoa.net/xml/VOEvent/v1.11"
	xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
	xmlns:lmsal="http://sot.lmsal.com/lmsal"
	xmlns:crd="urn:nvo-coords"
	xsi:schemaLocation="http://www.ivoa.net/xml/VOEvent/VOEvent-v1.1.xsd">


	<Who>
		<!-- Data pertaining to curation: observer, telescope, instrument, planner, tohbans, ... -->
		<Date>2008-02-08T16:44:36.000Z</Date>    <!-- Time VOEvent was generated. -->
		<PublisherID>http://sot.lmsal.com</PublisherID>

		<Contact>
			<Name>Ted Tarbell</Name>
			<Institution>LMSAL</Institution>
			<Communication>
				<Uri>http://lmsal.com</Uri>
				<AddressLine>3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA, 94304</AddressLine>
				<Telephone>+1-650-424-2400</Telephone>
				<Email>tarbell@lmsal.com</Email>
			</Communication>		</Contact>

		<lmsal:Telescope>Hinode</lmsal:Telescope>
		<lmsal:Instrument>SOT</lmsal:Instrument>
		<lmsal:Tohbans>Imada</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Sterling</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Cruz</lmsal:ChiefObserver>
	</Who>


	<What>
		<!-- Data pertaining to what was observed, measured, ...   Some of these tags might move into Who section. -->
		<lmsal:obsId></lmsal:obsId>
		<lmsal:OBS_NUM>61</lmsal:OBS_NUM>
		<lmsal:JOP_ID>61</lmsal:JOP_ID>
		<lmsal:JOP></lmsal:JOP>
		<lmsal:JOIN_SB>null</lmsal:JOIN_SB>    <!-- S=SOT, X=XRT, E=EIS, SX=SOT+XRT, EX=EIS+XRT -->
		<lmsal:OBSTITLE>EIS Near On-Disk CH Study</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>CH</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>CH</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM></lmsal:NOAA_NUM>
		<lmsal:TARGET>Coronal Hole</lmsal:TARGET>
		<lmsal:slotNumber>3</lmsal:slotNumber>
	</What>


	<WhereWhen>
		<!-- Space and Time Coordinates. -->
		<ObservatoryLocation ID="Hinode" />

		<ObservationLocation>
			<lmsal:xCen>685</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>-97</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2008-02-11T04:38:30.000Z 2008-02-11T10:14:00.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>685 -97</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2008-02-11T08:46:00Z 2008-02-11T09:07:30Z" />
			<Param name="saaInterval" value="2008-02-11T05:25:30Z 2008-02-11T05:53:30Z" />
			<Param name="saaInterval" value="2008-02-11T07:06:00Z 2008-02-11T07:31:00Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>CORE: Long Duration Studies of Equatorial Coronal Holes</lmsal:Goal>
			<lmsal:Purpose>Na IV,Ca,GB 4kx2k 2x2, 3 min low cadence</lmsal:Purpose>
		</Concept>

		<Description>
			This is a follow-on study to the investigations of Jets in polar coronal holes.  We propose to follow low latitude coronal holes from near disk center to the west limb. Combined SOT, XRT and EIS observations are needed near disk center to accurately measure the magnetic field evolution that leads to coronal jets and (with luck) the line-of-sight velocity of the jets in several lines. Following the CH from the disk to the limb will allow for detail comparison with the polar jets and at the limb. We will have joint observations with SOHO UVCS.  A primary goal is to observe to observe the jet from initiation through decay in all three Hinode instruments.
		</Description>
	</Why>

</VOEvent>
