Prediction of solar flare through sunspot digital optical observation
In this paper, we discuss about the prediction of solar flare through sunspot digital optical observation, based on 4 sets of H alpha archive data from the Big Bear Solar Observatory. The brightness and pattern of 3D surface plot of the sunspot areas are analyzed for a few hours before and after the...
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description | In this paper, we discuss about the prediction of solar flare through sunspot digital optical observation, based on 4 sets of H alpha archive data from the Big Bear Solar Observatory. The brightness and pattern of 3D surface plot of the sunspot areas are analyzed for a few hours before and after the eruption of solar flare. Results show that the sunspot areas are gradually merged and at its peak brightness before the eruption of solar flare. The possible cause of these two precursors of solar flare will then be discussed. |
doi_str_mv | 10.1063/1.4915181 |
format | Conference Proceeding |
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The brightness and pattern of 3D surface plot of the sunspot areas are analyzed for a few hours before and after the eruption of solar flare. Results show that the sunspot areas are gradually merged and at its peak brightness before the eruption of solar flare. The possible cause of these two precursors of solar flare will then be discussed.</description><identifier>ISSN: 0094-243X</identifier><identifier>EISSN: 1551-7616</identifier><identifier>DOI: 10.1063/1.4915181</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Brightness ; Solar flares ; Sunspots</subject><ispartof>AIP conference proceedings, 2015, Vol.1657 (1)</ispartof><rights>2015 AIP Publishing LLC.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>309,310,780,784,789,790,23928,23929,25138,27923</link.rule.ids></links><search><title>Prediction of solar flare through sunspot digital optical observation</title><title>AIP conference proceedings</title><description>In this paper, we discuss about the prediction of solar flare through sunspot digital optical observation, based on 4 sets of H alpha archive data from the Big Bear Solar Observatory. The brightness and pattern of 3D surface plot of the sunspot areas are analyzed for a few hours before and after the eruption of solar flare. Results show that the sunspot areas are gradually merged and at its peak brightness before the eruption of solar flare. The possible cause of these two precursors of solar flare will then be discussed.</description><subject>Brightness</subject><subject>Solar flares</subject><subject>Sunspots</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2015</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotjc1KAzEURoMoOFYXvkHA9dTcm99ZSqlWKOhCwV1JJpl2yjAZk4zPb4tuzlmd7yPkHtgSmOKPsBQNSDBwQSqQEmqtQF2SirFG1Cj41zW5yfnIGDZam4qs31PwfVv6ONLY0RwHm2h3QqDlkOK8P9A8j3mKhfp-3xc70DiVvj3b5ZB-7Dm9JVedHXK4-_eCfD6vP1abevv28rp62tYTSl5qDlJZIRT3XjkjhEMAzbX01qH10jcMvUO00rWoVOcby5wFLhqjULBg-II8_O1OKX7PIZfdMc5pPF3uEFAYFBqB_wKCK0vk</recordid><startdate>20150424</startdate><enddate>20150424</enddate><general>American Institute of Physics</general><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20150424</creationdate><title>Prediction of solar flare through sunspot digital optical observation</title></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p253t-3156a4463dd6b844b2117375dab2ad5d902db22a5bc266fd9a0ba134986240e83</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Brightness</topic><topic>Solar flares</topic><topic>Sunspots</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Prediction of solar flare through sunspot digital optical observation</atitle><btitle>AIP conference proceedings</btitle><date>2015-04-24</date><risdate>2015</risdate><volume>1657</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>In this paper, we discuss about the prediction of solar flare through sunspot digital optical observation, based on 4 sets of H alpha archive data from the Big Bear Solar Observatory. The brightness and pattern of 3D surface plot of the sunspot areas are analyzed for a few hours before and after the eruption of solar flare. Results show that the sunspot areas are gradually merged and at its peak brightness before the eruption of solar flare. The possible cause of these two precursors of solar flare will then be discussed.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4915181</doi></addata></record> |
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language | eng |
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source | AIP Journals Complete |
subjects | Brightness Solar flares Sunspots |
title | Prediction of solar flare through sunspot digital optical observation |
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