Jasinski, JM; Arridge, CS; Lamy, L; Leisner, JS; Thomsen, MF; Mitchell, DG; Coates, AJ; ... Waite, JH; + view all Jasinski, JM; Arridge, CS; Lamy, L; Leisner, JS; Thomsen, MF; Mitchell, DG; Coates, AJ; Radioti, A; Jones, GH; Roussos, E; Krupp, N; Grodent, D; Dougherty, MK; Waite, JH; - view fewer (2014) Cusp observation at Saturn's high-latitude magnetosphere by the Cassini spacecraft. GEOPHYSICAL RESEARCH LETTERS , 41 (5) 1382 - 1388. 10.1002/2014GL059319.

Preview

PDF grl51465.pdf Download (2MB)

Abstract

We report on the first analysis of magnetospheric cusp observations at Saturn by multiple in situ instruments onboard the Cassini spacecraft. Using this we infer the process of reconnection was occurring at Saturn’s magnetopause. This agrees with remote observations that showed the associated auroral signatures of reconnection. Cassini crossed the northern cusp around noon local time along a poleward trajectory. The spacecraft observed ion energy-latitude dispersions—a characteristic signature of the terrestrial cusp. This ion dispersion is “stepped,” which shows that the reconnection is pulsed. The ion energy-pitch angle dispersions suggest that the field-aligned distance from the cusp to the reconnection site varies between ∼27 and 51 RS. An intensification of lower frequencies of the Saturn kilometric radiation emissions suggests the prior arrival of a solar wind shock front, compressing the magnetosphere and providing more favorable conditions for magnetopause reconnection.

Download activity - last month

Export as XMLJSONCSV

Download activity - last 12 months

Export as XMLCSVJSON

Downloads by country - last 12 months

Export as JSONCSVXML

Archive Staff Only

View Item