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Titel Direct observations of blob deformation during a substorm
VerfasserIn T. Ishida, Y. Ogawa, A. Kadokura, K. Hosokawa, Y. Otsuka
Medientyp Artikel
Sprache Englisch
ISSN 0992-7689
Digitales Dokument URL
Erschienen In: Annales Geophysicae ; 33, no. 5 ; Nr. 33, no. 5 (2015-05-06), S.525-530
Datensatznummer 250121194
Publikation (Nr.) Volltext-Dokument vorhandencopernicus.org/angeo-33-525-2015.pdf
 
Zusammenfassung
Ionospheric blobs are localized plasma density enhancements, which are mainly produced by the transportation process of plasma. To understand the deformation process of a blob, observations of plasma parameters with good spatial–temporal resolution are desirable. Thus, we conducted the European Incoherent Scatter radar observations with high-speed meridional scans (60–80 s) during October and December 2013, and observed the temporal evolution of a blob during a substorm on 4 December 2013. This paper is the first report of direct observations of blob deformation during a substorm. The blob deformation arose from an enhanced plasma flow shear during the substorm expansion phase, and then the blob split into two smaller-scale blobs, whose scale sizes were more than ~100 km in latitude. Our analysis indicates that the Kelvin–Helmholtz instability and dissociative recombination could have deformed the blob structure.
 
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