An upper bound on the solar radar cross section at 50 MHz

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dc.contributor.authorColes, W.A.
dc.contributor.authorHarmon, J. K.
dc.contributor.authorSulzer, M. P.
dc.contributor.authorChau Chong Shing, Jorge Luis
dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.date.accessioned2018-07-16T15:54:17Z
dc.date.available2018-07-16T15:54:17Z
dc.date.issued2006-04
dc.description.abstractWe have made 16 unsuccessful attempts, in February and October 2003, and February 2004, to observe solar echoes using the 50 MHz radar at Jicamarca in Peru. The upper bound that we have determined on the solar cross section is significantly lower than the average of earlier reported observations. In this paper we will describe the observations, discuss the noise and interference from solar bursts, and suggest possible reasons why the echo might be weaker than expected.
dc.description.peer-reviewPor pares
dc.formatapplication/pdf
dc.identifier.citationColes, W. A., Harmon, J. K., Sulzer, M. P., Chau, J. L., & Woodman, R. F. (2006). An upper bound on the solar radar cross section at 50 MHz.==$Journal of Geophysical Research: Space Physics, 111$==(A4), A04102. https://doi.org/10.1029/2005JA011416
dc.identifier.doihttps://doi.org/10.1029/2005JA011416
dc.identifier.govdocindex-oti2018
dc.identifier.journalJournal of Geophysical Research: Space Physics
dc.identifier.urihttp://hdl.handle.net/20.500.12816/1884
dc.language.isoeng
dc.publisherAmerican Geophysical Union
dc.relation.ispartofurn:issn:2169-9380
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttps://creativecommons.org/licences/by/4.0/
dc.subjectRadar
dc.subjectSolar
dc.subjectEchoes
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01
dc.titleAn upper bound on the solar radar cross section at 50 MHz
dc.typeinfo:eu-repo/semantics/article

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