Occurrence Statistics of Horse Collar Aurora

نویسندگان

چکیده

Horse collar aurora (HCA) are an auroral feature where the dawn and dusk sector oval moves polewards polar cap becomes teardrop shaped. They form during prolonged periods of northward interplanetary magnetic field (IMF), when IMF clock angle is small. Their formation has been linked to dual-lobe reconnection (DLR) closing flux at dayside magnetopause. The conditions necessary for DLR currently not well-understood therefore understanding HCA statistics will allow be studied in more detail. We have identified over 600 events between 2010 2016 UV images captured by Special Sensor Ultraviolet Spectrographic Imager instrument on-board Defense Meteorological Satellite Program spacecraft F16, F17 F18. As expected, there a clear preference occurring IMF. find no seasonal dependence their occurrence, with average 8 per month. occurrence does appear depend on Bx component Considering radiance intensity across dusk-dawn meridian shows as separate bulge inside that side arc usually brighter than Lyman-Birge-Hopfield short band. relate this expected aligned current pattern formation. further suggest transpolar arcs observed simultaneously both northern southern hemispheres misidentified HCA.

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ژورنال

عنوان ژورنال: Journal Of Geophysical Research: Space Physics

سال: 2022

ISSN: ['2169-9402', '2169-9380']

DOI: https://doi.org/10.1029/2022ja030385