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<ri:Resource created="2000-02-28T18:56:36Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>The SMM Atlas of Gamma-Ray flares</title><shortName>J/ApJS/120/409</shortName><identifier>ivo://CDS.VizieR/J/ApJS/120/409</identifier><altIdentifier>doi:10.26093/cds/vizier.21200409</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vestrand W. T.</name></creator><creator><name>Share G. H.</name></creator><creator><name>Murphy R. J.</name></creator><creator><name>Forrest D. J.,Rieger E.</name></creator><creator><name>Chupp E. L.</name></creator><creator><name>Kanbach G.</name></creator><date role="Updated">2000-02-28T17:56:46Z</date><date role="Created">2000-02-28T18:56:36Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>star-atlases</subject><subject>gamma-ray-astronomy</subject><subject>solar-system</subject><description>We present a compilation of data for all 258 gamma-ray flares detected above 300 keV by the Gamma Ray Spectrometer (GRS) aboard the Solar Maximum Mission satellite. This gamma-ray flare sample was collected during the period from 1980 February to 1989 November; covering the latter half of the 21st solar sunspot cycle and the onset of the 22d solar sunspot cycle. We describe the SMM/GRS instrument, its in-orbit operation, and the principal data reduction methods used to derive the gamma-ray flare properties. Utilizing measurements for 185 flares that were sufficiently intense to allow the derivation of gamma-ray spectra, we present an atlas of time profiles and gamma-ray spectra. The flare parameters derived from the gamma-ray spectra include bremsstrahlung fluence and best-fit power-law parameters, narrow nuclear line fluence, positron annihilation line fluence, neutron capture line fluence, and an indication of whether or not emissions greater than 10 MeV were present. Since a uniform methodology was adopted for deriving the parameters, this atlas should be very useful for future statistical and correlative studies of solar flares.</description><source format="bibcode">1999ApJS..120..409V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/120/409</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/120/409</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/120/409</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/120/409</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/120/409</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/120/409</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/120/409</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><facility>SMM</facility><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/120/409/table1</name><description>Compilation of data for gamma-ray flares</description><column><name>Code</name><description>Event code (5)</description><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flare</name><description>Date of gamma-ray flare occurrence (year)</description></column><column><name>Durat</name><description>? Flare Duration</description><unit>s</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Pos</name><description>Position of associated H{alpha} flare</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Prop</name><description>Properties (1)</description><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Vangle</name><description>? Heliocentric viewing angle for the flare</description><unit>deg</unit><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Amp</name><description>? Amplitude of bremstahlung power-law measured at 0.3 MeV (photons.cm-2.s-1)</description><unit>cm**-2.s**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Amp</name><description>? errors of the Amplitude</description><unit>cm**-2.s**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Index</name><description>? Index of the best fit power-law</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Index</name><description>? errors of the index</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Tbrem</name><description>? Total bremsstrahlung fluence between 0.3-8.5 MeV (photons.cm-2)</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Tbrem</name><description>? errors of the bremsstrahlung fluence</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Tnuc</name><description>? Total narrow nuclear line fluence (photons.cm-2) (2)</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Tnuc</name><description>? errors of the nuclear fluence</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Posit</name><description>? Fluence of the 0.511 MeV line (photons.cm-2.s-1) (3)</description><unit>cm**-2.s**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Posit</name><description>? errors of the positron fluence</description><unit>cm**-2.s**-1</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ncap</name><description>? Fluence of the 2.23 MeV line (photons.cm-2.s-1) (4)</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ncap</name><description>? errors in the 2.23 MeV line</description><unit>cm**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>