Saturn kilometric radiation as a monitor for the solar wind?

Autor: Philippe Zarka, Mykhaylo Panchenko, David J. McComas, Patrick H. M. Galopeau, Mohammed Y. Boudjada, C. H. Barrow, Helmut O. Rucker, John T. Steinberg, Kirk C. Hansen, U. Taubenschuss, William S. Kurth, Michele K. Dougherty

Publikováno v: Advances in Space Research
Advances in Space Research, Elsevier, 2008, 42 (1), pp.40-47. ⟨10.1016/j.asr.2008.02.008⟩
Advances in Space Research, 2008, 42 (1), pp.40-47. ⟨10.1016/j.asr.2008.02.008⟩

Since the Voyager mission it is known that Saturn Kilometric Radiation (SKR) is strongly influenced by external forces, i.e., the solar wind and in particular the solar wind ram pressure. Recent studies using Cassini data essentially confirmed these

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9870242b32e0b49b97fe44771d4db680
https://doi.org/10.1016/j.asr.2008.02.008

Jovicentric latitude effect on the bKOM radio emission observed by Ulysses/URAP

Autor: C. H. Barrow, Robert J. MacDowall, Alain Lecacheux

Publikováno v: Astronomy & Astrophysics. 366:343-350

During 1994 and into 1996, Ulysses was at distances of 5 AU or more from Jupiter and travelling from south to north of the ecliptic plane. At these distances, the jovian broadband radio emission (bKOM) was only received occasionally by the Unied Radi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::51cbea116543ad42aeb5242d9eb42861
https://doi.org/10.1051/0004-6361:20000100

Radio observations of the Jovian magnetic field

Autor: C. H. Barrow, Thomas D. Carr

Publikováno v: Advances in Space Research. 12:155-164

Radio observations of Jupiter are reviewed and discussed in relation to the planet's magnetic field. Early ground-based decameter- and decimeter-wave observations lead to a first estimate of the magnetic field strength which was subsequently confirme

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::ae2d8596b2ff7889bfd6ebf20717857b
https://doi.org/10.1016/0273-1177(92)90388-e

Solar type III burst profiles at decametre-wave frequencies

Autor: C. H. Barrow, A. Achong

Publikováno v: Solar Physics. 45:467-476

Solar type III bursts have been observed at fixed frequencies of 18, 22, 26 and 36 MHz during the period 1970–1974. 103 profiles have been analyzed in the manner introduced by Aubier and Boischot (1972) whose results are generally confirmed. Averag

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::5d0687054abb3a6783c61e6ab176de61
https://doi.org/10.1007/bf00158463

X-ray and radio emissions in the early stages of solar flares

Autor: A. Raoult, C. H. Barrow, Monique Pick, A. O. Benz, Brian R. Dennis, G. M. Simnett

Publikováno v: Solar Physics. 83:267-283

Radio and X-ray observations are presented for three flares which show significant activity for several minutes prior to the main impulsive increase in the hard X-ray flux. The activity in this ‘pre-flash’ phase is investigated using 3.5 to 461 k

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::5f213b477e077efda768f4ee1ad92ea2
https://doi.org/10.1007/bf00148280