<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="prediction"
	ivorn="ivo://sot.lmsal.com/VOEvent#2016-08-19T16:00:00Z"
	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>2016-08-17T21:02:11.000Z</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>Arikawa</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Arikawa</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Cruz (RCO)-> Oba</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>320</lmsal:OBS_NUM>
		<lmsal:JOP_ID>320</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 320 w/IRIS, BBSO @ AR12578</lmsal:OBSTITLE>
		<lmsal:SCI_OBJ>AR</lmsal:SCI_OBJ>     <!--  Scientific objectives -->
		<lmsal:SCI_OBS>AR</lmsal:SCI_OBS>     <!-- Objects being observed -->
		<lmsal:NOAA_NUM>12578</lmsal:NOAA_NUM>
		<lmsal:TARGET>MicroFlare</lmsal:TARGET>
		<lmsal:slotNumber>15</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>-299</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>3</lmsal:yCen>
			<lmsal:xFov>0</lmsal:xFov>
			<lmsal:yFov>0</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2016-08-19T16:00:00.000Z 2016-08-19T17:20:30.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>-299 3</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

		<Group name="saaIntervals">
			<Param name="saaInterval" value="2016-08-19T16:57:00Z 2016-08-19T17:20:30Z" />
		</Group>
	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>Small-scale solar activities and their spectroscopic property</lmsal:Goal>
			<lmsal:Purpose>Normal map 82&quot;x82&quot;, Q65/Q75, 1 side</lmsal:Purpose>
		</Concept>

		<Description>
			abstract of observational proposal It is well accepted that the small-scale solar activities play important roles in heating the upper solar atmosphere, including the solar chromosphere and the solar corona (Li et al. 2007; Schmieder et al. 2013; Wang et al. 2014). Detailed study of the response of the upper solar atmosphere to small-scale flux emergence and the related changes of physical parameters will open a new window to investigate the heating mechanisms of the upper solar atmosphere. In this proposal, we would like to observe small-scale solar activities, such as small-scale emerging flux region (SEFR), Ellerman Bombs (EBs), jets, coronal bright points (CBPs) with the Interface Region Imaging Spectrometer (IRIS) together with Hinode and New Solar Telescope (NST) at Big Bear Solar Observatory (BBSO) in order to investigate the physical properties, spectroscopic characteristics and evolutions of these activities.   request to SOT SP, Normal map mode FOV: 82"?82" Time cadence: 43 min Duration: 7 hours Data volume: 2833 Mbits
		</Description>
	</Why>

</VOEvent>
