<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2019-09-27T14:00:00Z"
	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>2019-09-26T11:57:00.000Z</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>Brooks</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Tiwari and DeRosa (RCO) -> Hasegawa</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>373</lmsal:OBS_NUM>
		<lmsal:JOP_ID>373</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 373 filament @S40</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>7</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>113</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>-723</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2019-09-27T14:00:00.000Z 2019-09-27T14:56:00.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>113 -723</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2019-09-27T15:28:00Z 2019-09-27T15:39:30Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>Formation and destabilisation of filaments</lmsal:Goal>
			<lmsal:Purpose>Fast map, 230&quot;x164&quot;, Q65, 1-side CCD</lmsal:Purpose>
		</Concept>

		<Description>
			Main Objective: SOT/SP would measure the parasitic polarities in the barbs of filaments.  Scientific Justification: Filaments are formed with shear flows in channel. It will be interesting to detect the footpoints of  filament and  mass motions inside the barbs and along the filaments. Spectroscopic observations on the disk in  chromosphere lines (Mg II h and k, Halpha) and photosphere lines are required to show the dynamics of the filament by counter-streaming or by turbulence. HMI continua and magnetogram will provide data to follow the large scale  evolution of the channel. With HMI surface velocities by using CST (LCT)  methods  will  be determined leading to an  estimate of the shear at large scale of the filament and Hinode/SOT will locate the parasitic polarities where the filament has its footpoints.
		</Description>
	</Why>

</VOEvent>
