Premium
Periodicity in Saturn's magnetosphere: Plasma cam
Author(s) -
Burch J. L.,
DeJong A. D.,
Goldstein J.,
Young D. T.
Publication year - 2009
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2009gl039043
Subject(s) - plasmoid , magnetosphere , physics , saturn , magnetosphere of saturn , plasma , longitude , plasma sheet , spiral (railway) , astrophysics , ion , astronomy , magnetopause , planet , latitude , magnetic reconnection , nuclear physics , mathematical analysis , mathematics , quantum mechanics
Plasma ion data from the Cassini Plasma Spectrometer (CAPS) are examined for all orbits from October 25, 2004 through Dec. 26, 2007. To eliminate effects of incomplete angular coverage, data are only used from the CAPS anode that is closest to viewing into the corotational flow and within 20° of that flow. The data are plotted in the SKR‐based SLS3 longitude system. The result is a cam‐shaped distribution in radial distance and SLS3 that has an outer lobe extending beyond 20 R S at SLS3 longitudes in the range ∼270° − 50°. The western edge of this outer lobe maps to the inner extent of a previously observed spiral pattern of periodic ion enhancements, which had the magnetic signature of plasmoids at distances >35 Rs. The plasma cam and the plasmoid spiral emanating from it are responsible for plasma periodicities observed at radial distances beyond ∼15 Rs in Saturn's magnetosphere.