Back to results

Lancaster University

Solar wind-magnetosphere interactions : a statistical analysis of spacecraft measurements

Abstract

dc:description.abstract

When investigating solar wind-magnetosphere-ionosphere coupling, it is important to understand how the solar wind, and the interplanetary magnetic field (IMF) frozen into it, behaves as it reaches the Earth. Magnetic reconnection, for example, is a phenomenon whose morphology is governed by the IMF orientation and wields a large influence over many of the processes occurring within the magnetosphere. Exploiting nearly a decade of spacecraft data, primarily from ESA's Cluster mission and NASA's ACE mission, the three studies presented in this thesis aim to help improve the specification of the IMF at the magnetopause.

Degree

thesis:*
Name dc:type.qualificationname
Ph.D.
Level dc:type.qualificationlevel
doctoral
Grantor dc:publisher.institution
Lancaster University
Year dc:date.issued
2014

Author and committee

dc:creator, dc:contributor.*
Authors dc:creator
  • Case, Nathan
  • Wild, Jim

Chain of custody

source
Harvested from
Lancaster University
Base URL
eprints.lancs.ac.uk/cgi/oai2
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
related terms
citation

Case, Nathan; Wild, Jim. Solar wind-magnetosphere interactions : a statistical analysis of spacecraft measurements. doctoral thesis, Lancaster University, 2014.