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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_AU
dc.language.isoenen_AU
dc.rightsCreative Commons Attribution 4.0en_AU
dc.subjectradio emissionsen_AU
dc.subjectEarth's foreshocken_AU
dc.subjectshocksen_AU
dc.subjectspace plasma physicsen_AU
dc.subjectnonlinear wave-wave processesen_AU
dc.subjectlinear mode conversionen_AU
dc.titleOutput dataset for radio emission produced by the code hybrid_3DNov.m for standard parametersen_AU
dc.typeDataseten_AU
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5109 Space sciences::510902 Heliophysics and space weatheren_AU
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5106 Nuclear and plasma physics::510602 Plasma physics; fusion plasmas; electrical dischargesen_AU
dc.subject.asrcANZSRC FoR code::51 PHYSICAL SCIENCES::5101 Astronomical sciences::510108 Solar physicsen_AU
dc.relation.arcDP180103509
dc.relation.arcIC170100023
dc.description.methodOutput of the Matlab code hybrid_3DNov.m .en_AU
usyd.facultySeS faculties schools::Faculty of Science::School of Physicsen_AU
usyd.departmentARC Training Centre for CubeSats, UAVS, and Their Applications (CUAVA)en_AU
workflow.metadata.onlyNoen_AU


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