<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2008-08-07T22:34:00Z"
	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>2009-04-20T17:12:01.000Z</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>Arikawa</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Sterling</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>75</lmsal:OBS_NUM>
		<lmsal:JOP_ID>75</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>HOP 75 - N limb spicules</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>SPI</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>SPI</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM></lmsal:NOAA_NUM>
		<lmsal:TARGET>Spicule and Jets</lmsal:TARGET>
		<lmsal:slotNumber>7</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>0</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>923</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2008-08-07T22:34:00.000Z 2008-08-08T09:00:00.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>0 923</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2008-08-07T23:28:30Z 2008-08-07T23:46:30Z" />
			<Param name="saaInterval" value="2008-08-08T01:05:30Z 2008-08-08T01:12:30Z" />
			<Param name="saaInterval" value="2008-08-08T02:28:30Z 2008-08-08T02:48:30Z" />
			<Param name="saaInterval" value="2008-08-08T03:59:00Z 2008-08-08T04:25:30Z" />
			<Param name="saaInterval" value="2008-08-08T05:36:00Z 2008-08-08T06:03:00Z" />
			<Param name="saaInterval" value="2008-08-08T07:16:30Z 2008-08-08T07:40:30Z" />
			<Param name="saaInterval" value="2008-08-08T08:56:00Z 2008-08-08T09:00:00Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>Coordinated Observations between Hida Observatory and; Hinode Satellite</lmsal:Goal>
			<lmsal:Purpose>CaH 108x54&quot;&quot;, ROI 2, 2x2, 500ms, Q75</lmsal:Purpose>
		</Concept>

		<Description>
			HOP 75 has three targets in each three days; target 1 is a study of XBPs near DC with SOT 40 sec cadence data of Ca II H and NaD IandV, target 2 is polar X-ray jets and SOT provides 20 sec cadence data of Ca II H and NaD IandV, and target 3 is chromospheric jets in QS, SOT will give 10 sec cadence data of Ca II H and NaD IVDG. Scientific Objectives:  Chromospheric active phenomena, reconnections, coronal heating process and sunspot evolution that are all related with the solar magnetic field have become more clear by recent MHD simulations and high-resolution observations with the HINODE satellite.  We intend to quantitatively verify the present models of such phenomena by simultaneous and high-cadence observations of diversified observation from the photosphere to the corona with the HINODE satellite and spectrum observation at the Hida Obs.
		</Description>
	</Why>

</VOEvent>
