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dc.contributor.authorOppel, Patrick
dc.contributor.authorCairns, Iver
dc.date.accessioned2025-01-13T23:30:28Z
dc.date.available2025-01-13T23:30:28Z
dc.date.issued2025-01-14
dc.identifier.urihttps://hdl.handle.net/2123/33528
dc.description.abstractThis is an example output file of the code hybrid_3DNov.m for the "standard" case with 400km/s vsw and 60deg theta_bn (see input file init.m). This output is one of those presented in the Cairns and Oppel paper on images of Earth's foreshock radiation sources.en
dc.language.isoenen
dc.rightsCreative Commons Attribution 4.0en
dc.subjectradio emissionsen
dc.subjectEarth's foreshocken
dc.subjectshocksen
dc.subjectspace plasma physicsen
dc.subjectnonlinear wave-wave processesen
dc.subjectlinear mode conversionen
dc.titleOutput dataset for radio emission produced by the code hybrid_3DNov.m for standard parametersen
dc.typeDataseten
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5109 Space sciences::510902 Heliophysics and space weatheren
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5106 Nuclear and plasma physics::510602 Plasma physics; fusion plasmas; electrical dischargesen
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5101 Astronomical sciences::510108 Solar physicsen
dc.relation.arcDP180103509
dc.relation.arcIC170100023
dc.description.methodOutput of the Matlab code hybrid_3DNov.m .en
usyd.facultySeS faculties schools::Faculty of Science::School of Physicsen
usyd.departmentARC Training Centre for CubeSats, UAVS, and Their Applications (CUAVA)en
workflow.metadata.onlyNoen


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