{"id":463,"date":"2021-04-22T17:31:40","date_gmt":"2021-04-22T17:31:40","guid":{"rendered":"https:\/\/celestina.web.uah.es\/wordpress\/?page_id=463"},"modified":"2024-01-25T09:28:03","modified_gmt":"2024-01-25T09:28:03","slug":"data","status":"publish","type":"page","link":"https:\/\/celestina.web.uah.es\/wordpress\/en\/data\/","title":{"rendered":"Data"},"content":{"rendered":"\n

Data from the e-Callisto network radio telescopes is available in http:\/\/soleil.i4ds.ch\/solarradio\/callistoQuicklooks\/<\/a>. The data provided by celestina nodes can be found by searching for SPAIN-ALCALA, SPAIN-PERALEJOS and SPAIN-SIGUENZA. Light curves can be found be found in http:\/\/soleil.i4ds.ch\/solarradio\/data\/Lightcurves\/<\/a>. Below are the most recent light curves of CELESTINA nodes. In general, solar radio bursts have a Y-factor of 3 dB, so the level of interference at the radio telescope location must be below 3 dB in order to detect them. The province of Guadalajara offers such unique places, not only for its heritage or natural beauty, but for its low level of electromagnetic pollution.<\/p>\n\n\n\n

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burst_matrix_20241013.png<\/center>\n\t\t<\/div>
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Automatic Solar Burst Detection using IA<\/center><\/p>\n\n\n\n

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SPAIN-PERALEJOS_20260403_62.png<\/center>\n\t\t<\/div>
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Light Curve in Melibea-01 (Peralejos de las Truchas)<\/center><\/p>\n\n\n\n

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SPAIN-PERALEJOS_20260317_03.png<\/center>\n\t\t<\/div>
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Light Curve in Melibea-03 (Peralejos de las Truchas)<\/center><\/p>\n\n\n\n

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SPAIN-PERALEJOS_20250331_63.png<\/center>\n\t\t<\/div>
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Light Curve in Melibea-04 (Peralejos de las Truchas)<\/center><\/p>\n\n\n\n

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SPAIN-SIGUENZA_20260403_02.png<\/center>\n\t\t<\/div>
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Light Curve in Doncel (Sig\u00fcenza)<\/center><\/p>\n","protected":false},"excerpt":{"rendered":"

Data from the e-Callisto network radio telescopes is available in http:\/\/soleil.i4ds.ch\/solarradio\/callistoQuicklooks\/. The data provided by celestina nodes can be found by searching for SPAIN-ALCALA, SPAIN-PERALEJOS and SPAIN-SIGUENZA. Light curves can be found be found in http:\/\/soleil.i4ds.ch\/solarradio\/data\/Lightcurves\/. Below are the most recent light curves of CELESTINA nodes. In general, solar radio bursts have a Y-factor of […]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-463","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/pages\/463","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/comments?post=463"}],"version-history":[{"count":14,"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/pages\/463\/revisions"}],"predecessor-version":[{"id":740,"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/pages\/463\/revisions\/740"}],"wp:attachment":[{"href":"https:\/\/celestina.web.uah.es\/wordpress\/wp-json\/wp\/v2\/media?parent=463"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}