<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2007-04-03T17:49:42.819Z"
	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>2007-04-03T17:49:42.000Z</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>Katsukawa</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Okamoto, Sterling, Kamio, Katsukawa, Hara, Narukage</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Berger/Lites/Kubo</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>0</lmsal:OBS_NUM>
		<lmsal:JOP_ID>0</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>Synoptic</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>DC, SYN</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>DC, SYN</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM></lmsal:NOAA_NUM>
		<lmsal:TARGET>Sun Center</lmsal:TARGET>
		<lmsal:slotNumber>4</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>0</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>0</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2007-03-11T18:03:30.000Z 2007-03-11T18:14:00.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>0 0</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>Synoptic; DC, SYN; Sun Center</lmsal:Goal>
			<lmsal:Purpose>Synoptic BFI NFI</lmsal:Purpose>
		</Concept>

		<Description>
			XRT: table uplead and memory dump of E2P ROM (in this week). X-ray Bright Point study if QS targets appropriate. andnbsp;  SOT: Irradiance Synoptic program with N/S scan with 13 pointings and activity belt scan of more than 13 pointings. Sekii-san's proposal on meridional flow study will be run. Shimda's sunspot program. Some additional flat fields will be run as well. Bruce Lite's 45 degree SP program  EIS: Active Region coronal loop studies are a high priority if a suitable target appears i.e. not just any active region but one with well defined loops, or a loop arcade, especially andnbsp;if it is close to the central meridian.   Other active region raster/slit observations requested but on any region at any time.   Request for some limb observations, perhaps after the activity belt scan is complete (i.e. stay at the limb afterwards)?   Will try to support irradiance program, probably with raster scans.
		</Description>
	</Why>

</VOEvent>
