Simulations of radio-wave anisotropic scattering to interpret type III radio bursts measurements by Solar Orbiter, Parker Solar Probe, STEREO and Wind

Simple item page
dc.contributor.authorMusset, S.
dc.contributor.authorMaksimovic, M.
dc.contributor.authorKontar, E.
dc.contributor.authorKrupar, V.
dc.contributor.authorChrysaphi, N.
dc.contributor.authorBonnin, X.
dc.contributor.authorVecchio, A.
dc.contributor.authorCecconi, B.
dc.contributor.authorZaslavsky, A.
dc.contributor.authorIssautier, K.
dc.contributor.authorBale, S. D.
dc.contributor.authorPulupa, M.
dc.date.accessioned2021-10-22T16:45:42Z
dc.date.available2021-10-22T16:45:42Z
dc.date.issued2021-09-29
dc.description.abstractWe use multi-spacecraft observations of invididual type III radio bursts in order to calculate the directivity of the radio emission, to be compared to the results of ray-tracing simulations of the radio-wave propagation and probe the plasma properties of the inner heliosphere. Ray-tracing simulations of radio-wave propagation with anisotropic scattering on density inhomogeneities are used to study the directivity of radio emissions. Simultaneous observations of type III radio bursts by four widely-separated spacecraft are used to calculate the directivity and position of the radio sources. The shape of the directivity pattern deduced for individual events is compared to the directivity pattern resulting from the ray-tracing simulations. We show that simultaneous observations of type radio III bursts by 4 different probes provide the opportunity to estimate the radio source positions and the directivity of the radio emission. The shape of the directivity varies from one event to another, and is consistent with anisotropic scattering of the radio-waves.en_US
dc.description.sponsorshipSolar Orbiter is a space mission of international collaboration between ESA and NASA, operated by ESA. Parker Solar Probe was designed, built, and is now operated by the Johns Hopkins Applied Physics Laboratory as part of NASA’s Living with a Star (LWS) program (contract NNN06AA01C). Support from the LWS management and technical team has played a critical role in the success of the Parker Solar Probe mission. The Wind/WAVES investigation is a collaboration of the Observatoire de Paris, NASA/GSFC, and the University of Minnesota. S. Musset is supported by an ESA Research Fellowship. V. Krupar acknowledges the support by NASA under grants 18-2HSWO218_2-0010 and 19-HSR-19_2-0143. N. Chrysaphi thanks CNES for its financial support. Data analysis was performed using IDL (Exelis Visual Information Solutions, Boulder, Colorado).en_US
dc.description.urihttps://www.aanda.org/articles/aa/pdf/forth/aa40998-21.pdfen_US
dc.format.extent9 pagesen_US
dc.genrejournal articlesen_US
dc.genrepreprintsen_US
dc.identifierdoi:10.13016/m2jqws-lwvt
dc.identifier.citationMusset, S. et al.; Simulations of radio-wave anisotropic scattering to interpret type III radio bursts measurements by Solar Orbiter, Parker Solar Probe, STEREO and Wind; Astronomy & Astrophysics, 29 September, 2021; https://doi.org/10.1051/0004-6361/202140998en_US
dc.identifier.urihttp://hdl.handle.net/11603/23149
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202140998
dc.language.isoen_USen_US
dc.publisherEDP Sciencesen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en_US
dc.rights©ESO 2021
dc.titleSimulations of radio-wave anisotropic scattering to interpret type III radio bursts measurements by Solar Orbiter, Parker Solar Probe, STEREO and Winden_US
dc.typeTexten_US

Files

Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
2109.13713.pdf
Size:
2.19 MB
Format:
Adobe Portable Document Format
Description:
Download
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
2.56 KB
Format:
Item-specific license agreed upon to submission
Description:
Download

Collections

UMBC Goddard Planetary Heliophysics Institute (GPHI)
UMBC Faculty Collection