Observations of the 2024 May 14 X8.7 Solar Flare with the Goldstone- Apple Valley Radio Telescope (GAVRT)
收藏DataCite Commons2024-06-17 更新2025-04-16 收录
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http://dataverse.jpl.nasa.gov/citation?persistentId=doi:10.48577/jpl.MVOXRE
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The Goldstone-Apple Valley Radio Telescope (GAVRT) project conducts a regular monitoring program of the Sun. GAVRT Solar Patrol project, uses a 34 m diameter antenna to produce raster-scan maps of the Sun simultaneously at 4 frequencies ranging from approximately 3 GHz to 14 GHz. On 2024 May 14, as part of regular GAVRT Solar Patrol observations, raster maps were produced when an X8.7 solar flare occurred in AR13664. AR13664 has reappeared as AR13697 and continues to be active producing X flares and GAVRT is monitoring its activity. Here we present the GAVRT maps of the May 14 X flare along with its microwave flux density spectra, showing the non-thermal microwave burst emission from mildly relativistic electrons produced in this largest flare of SC25 to date.
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2024-06-17



