<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2023-05-10T08:00:00Z"
	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>2023-05-08T20:45:27.000Z</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>Kotanagi</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Sakao</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>401</lmsal:OBS_NUM>
		<lmsal:JOP_ID>401</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>Coordination with SST and IRIS - Dynamics of flux cancellation in neutral lines</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>AR</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>AR</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM>13296</lmsal:NOAA_NUM>
		<lmsal:TARGET>Active Region</lmsal:TARGET>
		<lmsal:slotNumber>10</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>559</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>217</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2023-05-10T08:00:00.000Z 2023-05-10T08:47:30.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>559 217</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2023-05-10T08:26:00Z 2023-05-10T08:49:00Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>Dynamics of flux cancellation in neutral lines</lmsal:Goal>
			<lmsal:Purpose>Very Fast Map, 23x82&quot;, 1-side, repeat</lmsal:Purpose>
		</Concept>

		<Description>
			abstract of observational proposal Scientific Justification: The investigation focuses on the physics of flux cancellation in neutral lines. Reconnection events along neutral lines form the photosphere to higher heights in the atmosphere are believed to be behind the formation of filament channels, the seeds of CMEs. A large number of cancellation events in coordination with SST (Halpha - looking for heating events such as Ellerman bombs) is needed to elucidate the physical processes behind the creation of filament channels.   request to SOT Similar to HOP330 on 2017 April 22 at 14UT, but twice as wide (i.e. 20").
		</Description>
	</Why>

</VOEvent>
