<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2007-11-13T00:47:00Z"
	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>2009-03-13T15:12:54.000Z</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>Hara</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>27</lmsal:OBS_NUM>
		<lmsal:JOP_ID>27</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>HOP27 filament</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>FIL</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>FIL</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM></lmsal:NOAA_NUM>
		<lmsal:TARGET>Filament</lmsal:TARGET>
		<lmsal:slotNumber>5</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>-305</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>-548</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2007-11-13T00:47:00.000Z 2007-11-13T05:06:00.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>-305 -548</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2007-11-13T01:55:00Z 2007-11-13T02:13:00Z" />
			<Param name="saaInterval" value="2007-11-13T03:29:00Z 2007-11-13T03:50:00Z" />
			<Param name="saaInterval" value="2007-11-13T04:59:00Z 2007-11-13T05:06:00Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>SUMER campaign- 1. Temperature, density and 3-D structure of active region loops, 2. Chromospheric heating [SUMER #5]</lmsal:Goal>
			<lmsal:Purpose>Na IV,Ca,BC 2kx2k 2x2 (3min)</lmsal:Purpose>
		</Concept>

		<Description>
			--SUMER Campaign--- HOP27: 3-D Structure and Evolution of Filaments/Prominences (TUE 11/13: 0016 - 0500) HOP27 filament   2007/11/13 00:16:00 - 2007/11/13 04:59:35   pointing: (-305,-548)     FG07 (0x0175) Na IV 512x2k,Ca,BC 1kx2k 2x2 (20s)     SP01 (0x0038) Fast map 10x164"" 120 sec     FG05 (0x0173) Na IV,Ca,BC 2kx2k 2x2 (3min) Request to SOT HOP Number 0027   1. Hinode/SOT: NFI - Mg I Dopplergrams, magnetic field (2kx2k) - Mg Ib IVDG,          BFI: - Ca II (2kx2k), occasional G-band         SP: Sequence will depend on the target. Will use combination of          (a) fast mode (10""x164""), with repeat, 2 min cadence              (See 17:00 10/04/07)          (b) fast mode map (164""x164""). 2. Hinode/SOT: Ca II, Blue continuum (2kx2k), Fe I magnetic field        SP and;#8211; fast mode map (10hx164g) with repeat, 2 min cadence,           fast mode map (100hx164h) Scientific Objectives:  1. Scientific Objective: The aim is to simultaneously determine the 3-D geometric structure, temperature, density and flows of active region loops.  2.  The goal of this proposal is to determine the heating associated with specific magnetic field structure or magnetic field evolution.
		</Description>
	</Why>

</VOEvent>
