The University of Southampton
University of Southampton Institutional Repository

Magnetic reconnection in Saturn's magnetotail: a comprehensive magnetic field survey

Smith, A.W., Jackman, C.M. and Thomsen, M.F. (2016) Magnetic reconnection in Saturn's magnetotail: a comprehensive magnetic field survey Journal of Geophysical Research: Space Physics, n1-22. (doi:10.1002/2015JA022005).

Record type: Article


Reconnection within planetary magnetotails is responsible for locally energizing particles and changing the magnetic topology. Its role in terms of global magnetospheric dynamics can involve changing the mass and flux content of the magnetosphere. We have identified reconnection related events in spacecraft magnetometer data recorded during Cassini's exploration of Saturn's magnetotail. The events are identified from deflections in the north-south component of the magnetic field, significant above a background level. Data were selected to provide full tail coverage, encompassing the dawn and dusk flanks as well as the deepest midnight orbits. Overall 2094 reconnection related events were identified, with an average rate of 5.0 events per day. The majority of events occur in clusters (within 3 h of other events). We examine changes in this rate in terms of local time and latitude coverage, taking seasonal effects into account. The observed reconnection rate peaks postmidnight with more infrequent but steady loss seen on the dusk flank. We estimate the mass loss from the event catalog and find it to be insufficient to balance the input from the moon Enceladus. Several reasons for this discrepancy are discussed. The reconnection X line location appears to be highly variable, though a statistical separation between events tailward and planetward of the X line is observed at a radial distance of between 20 and 30RS downtail. The small sample size at dawn prevents comprehensive statistical comparison with the dusk flank observations in terms of flux closure.

Other jgra52493.pdf_v=1&t=inbodudf&s=2c0822936e9c43bc278c00b6f219671c28744a7d - Version of Record
Available under License Creative Commons Attribution.
Download (2MB)

More information

Accepted/In Press date: 3 March 2016
e-pub ahead of print date: 9 March 2016
Organisations: Astronomy Group


Local EPrints ID: 393267
ISSN: 2169-9380
PURE UUID: b3699b2d-b2b8-4325-a66d-cbe678c2a6b3
ORCID for A.W. Smith: ORCID iD

Catalogue record

Date deposited: 25 Apr 2016 11:16
Last modified: 17 Jul 2017 19:09

Export record



Author: A.W. Smith ORCID iD
Author: C.M. Jackman
Author: M.F. Thomsen

University divisions

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton:

ePrints Soton supports OAI 2.0 with a base URL of

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.