<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2019-09-04T12:00:00Z"
	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>2019-09-02T19:41:10.000Z</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>Yoshitake</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Yoshitake</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Cruz (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>384</lmsal:OBS_NUM>
		<lmsal:JOP_ID>384</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 384 with GREGOR</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>AR</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>AR</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM>12748</lmsal:NOAA_NUM>
		<lmsal:TARGET>Quiet Sun</lmsal:TARGET>
		<lmsal:slotNumber>2</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>123</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>55</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2019-09-04T12:00:00.000Z 2019-09-04T15:49:35.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>123 55</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2019-09-04T19:52:30Z 2019-09-04T20:15:30Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>The role of vertical magnetic fields in active regions</lmsal:Goal>
			<lmsal:Purpose>HOP 364 Normal Map, 123&quot;x123&quot;, 1-side, Q75</lmsal:Purpose>
		</Concept>

		<Description>
			Parker Solar Probe (PSP) will provide unprecedented observations of the conditions in the inner heliosphere. Remote sensing observations from EIS, XRT, SOT, and IRIS are needed to help identify and understand the solar origin of the plasma that PSP is observing.   Request to SOT HOP Number 0384    SOT-SP is required. Normal mode maps. FoV of 164" x 164"   Other Instruments:  GREGOR   Scientific Objectives:  Main Objective: To analyse the vertical component of the vector magnetic field in active regions. To study the evolution of the magnetic properties on the boundary of pores and umbrae, if any.
		</Description>
	</Why>

</VOEvent>
