<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2015-05-12T17:54:00Z"
	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>2015-05-18T18:24:26.000Z</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>Demoto</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Demoto</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>DeRosa (RCO)</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>19</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>2015-05-12T17:54:00.000Z 2015-05-12T17:57:00.000Z</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</lmsal:Goal>
			<lmsal:Purpose>Synoptic BFI NFI (revised:  small, no mask, Na D cont.)</lmsal:Purpose>
		</Concept>

		<Description>
			The immediate objective of these observations is the measurement of magnetic fields in prominences, solar tornados and/or spicules. We propose to exploit the excellent spectro-polarimetric capabilities of THEMIS for measurements of the magnetic field vector in prominences, solar tornadoes and spicules employing the inversions of the He D3 line. These phenomena represent unique examples of the small-scale coupling between magnetic field and plasma in environments with distinct dynamical behaviour. As such they represent key study-cases for deepening of our understanding of the Sun. SOT is used to give context to EIS and ease co-alignment with THEMIS.
		</Description>
	</Why>

</VOEvent>
