The Detectability of Radio Auroral Emission from Proxima B
The Detectability of Radio Auroral Emission from Proxima B
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Magnetically active stars possess stellar winds whose interaction with planetary magnetic fields produces radio auroral emission. We examine the detectability of radio auroral emission from Proxima b, the closest known exosolar planet orbiting our nearest neighboring star, Proxima Centauri. Using the Radiometric Bode's Law, we estimate the radio fl...
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Full title
The Detectability of Radio Auroral Emission from Proxima B
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TN_cdi_proquest_journals_2076634891
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076634891
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1706.07038
