In this section
@article{Carbary:2018:10.1002/2018GL077656,
author = {Carbary, JF and Mitchell, DG and Kollmann, P and Krupp, N and Roussos, E and Dougherty, MK},
doi = {10.1002/2018GL077656},
journal = {Geophysical Research Letters},
pages = {2911--2917},
title = {Energetic electron pitch angle distributions during the Cassini final orbits},
url = {http://dx.doi.org/10.1002/2018GL077656},
volume = {45},
year = {2018}
}
TY - JOUR
AB - Pitch angle distributions (PADs) of very energetic electrons (110–365 keV) are examined during the ringgrazing and proximal orbits of the Cassini spacecraft, from day 320 2016 (15 November) to day 257 2017 (14 September). These repeating orbits allowed a statistical evaluation of the PADs within the magnetopause on the nightside of Saturn. Along Lshells (i.e., equatorial crossing distances of magnetic field lines) near and outside that of Titan and north of the equator, the electron fluxes were unidirectionally fieldaligned going away from Saturn. Along Lshells inside Titan's and south of the equator, the electrons had bidirectional or pancake (trapping) PADs. This behavior suggests that the field lines within Titan's Lshell are generally closed, while those outside of that Lshell are generally open. This result strictly applies only to the nightside local times sampled during the final Cassini orbits, but one may infer a similar behavior at other times.
AU - Carbary,JF
AU - Mitchell,DG
AU - Kollmann,P
AU - Krupp,N
AU - Roussos,E
AU - Dougherty,MK
DO - 10.1002/2018GL077656
EP - 2917
PY - 2018///
SN - 0094-8276
SP - 2911
TI - Energetic electron pitch angle distributions during the Cassini final orbits
T2 - Geophysical Research Letters
UR - http://dx.doi.org/10.1002/2018GL077656
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000435743400004&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - http://hdl.handle.net/10044/1/63389
VL - 45
ER -