Frequency-Agile Solar Radiotelescope
Frequency-Agile Solar Radiotelescope (FASR) is a proposed next-generation radio telescope for solar observation in radio and microwave frequency range. In contrast to other general-purpose radio telescopes, such as the Very Large Array, FASR is specifically designed for solar observations. Compared with other astronomical sources, radio emission from the sun is highly time variable and the range of emission is very high.
Frequency-Agile Solar Radiotelescope
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- United States
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Frequency-Agile Solar Radiotelescope (FASR) is a proposed next-generation radio telescope for solar observation in radio and microwave frequency range. In contrast to other general-purpose radio telescopes, such as the Very Large Array, FASR is specifically designed for solar observations. Compared with other astronomical sources, radio emission from the sun is highly time variable and the range of emission is very high.
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wikidata · Q5502838 · wikipedia · Frequency-Agile Solar Radiotelescope
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The construction site of FASR is not yet determined but it will be somewhere in the southwest United States, as is its predecessor EOVSA
Frequency-Agile Solar Radiotelescope is associated with United States.
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- United States
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- arXiv, Cornell University, preprints naming “Frequency-Agile Solar Radiotelescope”
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- “Frequency-Agile Solar Radiotelescope”, English Wikipedia, consulted as further reading
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- Wikidata, structured authority record Q5502838: Frequency-Agile Solar Radiotelescope
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arXiv, Cornell University, preprints naming “Frequency-Agile Solar Radiotelescope”arXiv (Cornell University)
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The Encyclopedia exists whether or not anything is for sale. Corrections are recorded rather than overwritten, and every version of this record is kept. Published 16 August 2026.
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