Cusp observation at Saturn's high‐latitude magnetosphere by the Cassini spacecraft. Issue 5 (10th March 2014)

• Record Type: Journal Article
• Authors: Jasinski, J. M.; Arridge, C. S.; Lamy, L.; Leisner, J. S.; Thomsen, M. F.; Mitchell, D. G.; Coates, A. J.; Radioti, A.; Jones, G. H.; Roussos, E.; Krupp, N.; Grodent, D.; Dougherty, M. K.; Waite, J. H.
• Is Part Of: Geophysical research letters. Volume 41:Issue 5(2014:Mar.)
• Page Start: 1382
• Page End: 1388
• Publication Date: 2014-03-10
• Subjects: Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2014GL059319
• Languages: English
• ISSNs: 0094-8276

Abstract

<abstract abstract-type="main" id="grl51465-abs-0001"> <title> <x xml:space="preserve">Abstract</x> </title> <p id="grl51465-para-0001">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 <italic>R</italic>_{<italic>S</italic>}. 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.</p> </abstract>