UNDERSTANDING ION SPECTRAL DYNAMICS NEAR THE INNER EDGE OF THE PLASMA SHEET
type: CreativeWork
description: The inner magnetosphere is a highly dynamic space environment in which particles strongly interact with the magnetic and electric fields. During the last few decades, several missions have recorded the presence of dynamic spectral features of energetic ions in in situ measurements, which represent the observational signatures of ion transport, acceleration, and loss in the inner magnetosphere. These ion spectral features constitute the inner extent of access of the plasma sheet to the low L values and play an important role in the dynamics of the inner magnetosphere, yet no statistical results of their species dependence are available to date. This dissertation aims to examine the species dependence and preferred conditions for the formation of one type of ion spectral feature, the so-called nose structure. To achieve this objective, the research work combines extensive data analysis of ion flux measurements and numerical modeling of the observed spectral features. The spatial distribution, and dependence on energy, geomagnetic activity, and ion species (H+, He+, and O+) are established through large-scale statistical studies of ion nose structures using measurements from the Cluster and Van Allen Probes missions. To gain physical insight into the main observational results, these are interpreted employing numerical modeling of ion drift under a steady-state convection model with losses due to charge exchange. Moreover, the characteristics of ion noses during geomagnetic storms and the exact formation mechanism of multiple-nose structures are addressed for the first time in a case study of the geomagnetic storm of 2 October 2013. Van Allen Probes observations over the storm and simulations using a time-dependent convection model reveal the cyclic pattern of the storm-time nose structures. Furthermore, a detailed examination of the drift trajectories of ions composing multiple noses shows that multiple noses are formed by ions with resonant energies and whose traject…
abstract: The inner magnetosphere is a highly dynamic space environment in which particles strongly interact with the magnetic and electric fields. During the last few decades, several missions have recorded the presence of dynamic spectral features of energetic ions in in situ measurements, which represent the observational signatures of ion transport, acceleration, and loss in the inner magnetosphere. These ion spectral features constitute the inner extent of access of the plasma sheet to the low L values and play an important role in the dynamics of the inner magnetosphere, yet no statistical results of their species dependence are available to date. This dissertation aims to examine the species dependence and preferred conditions for the formation of one type of ion spectral feature, the so-called nose structure. To achieve this objective, the research work combines extensive data analysis of ion flux measurements and numerical modeling of the observed spectral features. The spatial distribution, and dependence on energy, geomagnetic activity, and ion species (H+, He+, and O+) are established through large-scale statistical studies of ion nose structures using measurements from the Cluster and Van Allen Probes missions. To gain physical insight into the main observational results, these are interpreted employing numerical modeling of ion drift under a steady-state convection model with losses due to charge exchange. Moreover, the characteristics of ion noses during geomagnetic storms and the exact formation mechanism of multiple-nose structures are addressed for the first time in a case study of the geomagnetic storm of 2 October 2013. Van Allen Probes observations over the storm and simulations using a time-dependent convection model reveal the cyclic pattern of the storm-time nose structures. Furthermore, a detailed examination of the drift trajectories of ions composing multiple noses shows that multiple noses are formed by ions with resonant energies and whose traject…
author: Ferradas, Cristian
keywords: Ions, Magnetosphere, Plasma sheet, Plasma transport, Ring Current, Space Physics, Geophysics, Plasma physics, Astrophysics
date published: 2017-01-01T08:00:00Z
date modified: 2026-07-24T05:22:01Z
provider: University of New Hampshire
publisher: Networked Digital Library of Theses and Dissertations
type: WebPage
source organization: University of New Hampshire