<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2008-01-05T09:10:00Z"
	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>2009-04-20T11:22:20.000Z</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>SOTSP</lmsal:Instrument>
		<lmsal:Tohbans>Bando</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Sakao</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Suematsu</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>62</lmsal:OBS_NUM>
		<lmsal:JOP_ID>62</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>HOP62 coronal thermal structure</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>CORE: Thermal distributions and evolutions of coronal structures</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>AR, SS</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM>10980</lmsal:NOAA_NUM>
		<lmsal:TARGET>Active Region</lmsal:TARGET>
		<lmsal:slotNumber>6</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>-463</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>-90</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2008-01-05T09:10:00.000Z 2008-01-05T10:51:35.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>-463 -90</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2008-01-07T08:14:00Z 2008-01-07T08:36:30Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>CORE: Thermal distributions and evolutions of coronal structures</lmsal:Goal>
			<lmsal:Purpose>Fast Map, Full FOV</lmsal:Purpose>
		</Concept>

		<Description>
			No specific request to SOT.  Scientific Objectives:  XRT has the capability for thermal studies using multi-filter observation sequences. Some multi-filter observations have been performed to-date, but the XRT Team would like to perform some coordinated observations with EIS and SOT. The primary science objective is study the thermal distribution and evolution of loop structures in active regions as well as XBPs, and cooler coronal structures, as seen by XRT and EIS rasters. (For example, some initial results by Reeves et al. directly show the spatial and thermal distribution of cooling plasma throughout coherent post-flare loop structures.)
		</Description>
	</Why>

</VOEvent>
