<?xml version="1.0" encoding="UTF-8" ?>
<VOEvent role="utility"
	ivorn="ivo://sot.lmsal.com/VOEvent#VOEvent_ObsS2007-08-23T07:05:50.000.xml"
	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>2007-08-23T16:13:52.000Z</Date>    <!-- Time VOEvent was generated. -->
		<PublisherID>http://sot.lmsal.com</PublisherID>

		<Contact>
			<Name>Mr. Sam Freeland</Name>
			<Institution>Lockheed Martin Solar and Astrophysics Laboratory (LMSAL)</Institution>
			<Communication>
				<Uri>http://www.lmsal.com</Uri>
				<AddressLine>Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304</AddressLine>
				<Telephone>null</Telephone>
				<Email>null</Email>
			</Communication>		</Contact>

		<lmsal:Telescope>HINODE</lmsal:Telescope>
		<lmsal:Instrument>SOT</lmsal:Instrument>
		<lmsal:Tohbans>Arikawa</lmsal:Tohbans>
		<lmsal:ChiefPlanner>Bando</lmsal:ChiefPlanner>
		<lmsal:ChiefObserver>Kubo</lmsal:ChiefObserver>
	</Who>


	<What>
		<!-- Data about what was measured/observed.  Some tags come from predicted event. -->
		<Param name="URLParent" value="http://www.lmsal.com/solarsoft/hinode/movies/voevent_movies_sot/2007/08/23/20070823_0000_20070824_0000_prog_15/20070823_0000_20070824_0000_prog_15.html" />
		<Param name="catalogLink" value="http://www.lmsal.com/cgi-ssw/sot_time2form.sh?start_time=2007-08-23+07%3A05%3A50.000&amp;amp;stop_time=2007-08-23+08%3A37%3A23.000&amp;amp;obs_type=*" />
		<lmsal:JOP_ID>20</lmsal:JOP_ID>
		<lmsal:OBSTITLE>EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating</lmsal:OBSTITLE>
		<lmsal:TARGET>coronal heating</lmsal:TARGET>
		<lmsal:SCI_OBJ>MFL</lmsal:SCI_OBJ>
		<lmsal:SCI_OBS>MFL</lmsal:SCI_OBS>
		<lmsal:NOAA_NUM>10969</lmsal:NOAA_NUM>
		<lmsal:slotNumber>15</lmsal:slotNumber>
	</What>


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

		<ObservationLocation>
			<lmsal:xCen>-459</lmsal:xCen>		<!-- xcen and ycen from FITS -->
			<lmsal:yCen>-240</lmsal:yCen>
			<lmsal:xFov>163</lmsal:xFov>
			<lmsal:yFov>163</lmsal:yFov>
			<crd:AstroCoords coord_system_id="UTC-HGS-TOPO">
				<crd:Time>
					<crd:TimeInterval>2007-08-23T07:05:50.000Z 2007-08-23T08:37:23.000Z</crd:TimeInterval>
				</crd:Time>
				<crd:Position3D>-459 -240</crd:Position3D>
			</crd:AstroCoords>
		</ObservationLocation>

	</WhereWhen>


	<Why>
		<!-- Why was observation performed.  Initial scientific assessment, hypothesized mechanisms, classifications, ... -->
		<Concept>
			<lmsal:Goal>EIS+ SOT+XRT Physical mechanisms driving solar microflares and supergranular network dynamics - relevance for coronal heating</lmsal:Goal>
			<lmsal:Purpose>w/s ShIV, CaH, G-b 2kx2k 2x2 1 min Q75</lmsal:Purpose>
		</Concept>

		<Description>
			Daily Note and User Entry:  HOP20: solar microflares and supergranular network dynamics (SOT/XRT/EIS) (07:00 - 13:30 UT)  EIS requests extended E/W limb observations for velocity calibration sometime this week (TBD). andnbsp;Target of opportunity observations of coronal hole on disk.  XRT: CCD Bakeout plus test X-ray images  SOT: Support HOP 20 07:00-13:30 UT; Request to SOT:  SOT: We plan (if possible) to run in time a sequence of 3exposures:2using the BFI imager and 1 using the NBIimager.The reason is to cover evolution of the photosphere with its magnetic concentration signatures (G-band), evolution of the longitudinal component of the magnetic field vector inthe photosphere, and evolution of chromosphere (CaIIH)witha reasonable temporal resolution (???"10s per image,???@???"30s???@per???@sequence???@of 3 selected channels).???@ ???@and;#8226;BFI: G-band and CaIIH channels, ???@ ;FOV:109???hx109???h(1k x1kmode, binning 2 x 2 pxs),  ; ;3bit JPEG compression, cadence:???"10s per filtergram,  ; ;telemetry needed: 300kbps, nocompensation of the solar rotation  ;and;#8226;NFI: FeI630.25nm longitudinal magnetograms,other parameters as in  ; ;case of BFI  ;and;#8226;SP:none; Scientific Objectives:  This proposal merges together attempts to observe two kinds of solarstructures and;#8211; solar micro flares and super granular network and;#8211; which are planned tobe investigated toaddress common openquestions on the irrelevance for the heating and dynamics of the solar corona.; Other Instruments:  DOT SoHO/CDS/MDI/EIT JOP 189: 3-17 Aug 2007 7:00 - 13:30 UT TRACE RHESSI
		</Description>
	</Why>

	<Citations>
	</Citations>
</VOEvent>
