Use this URL to cite or link to this record in EThOS: https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.771813
Title: Effects of field-aligned currents in the ionosphere-thermosphere system
Author: Hood, Rosie K. E.
ISNI:       0000 0004 7659 9419
Awarding Body: UCL (University College London)
Current Institution: University College London (University of London)
Date of Award: 2018
Availability of Full Text:
Access from EThOS:
Full text unavailable from EThOS. Please try the link below.
Access from Institution:
Abstract:
Space weather is one of the most significant natural hazards to modern day civilisation, posing a risk to both space and ground infrastructure. It describes the near-Earth and terrestrial environment as affected by the Sun, namely as a result of radiation, interactions with the interplanetary magnetic field and plasma outflow, the latter termed the solar wind. Field-aligned currents (FACs), that is, solar wind-driven currents aligned with the Earth's geomagnetic field and closed in its ionosphere, play an essential role in the transfer of energy and circulation between the solar wind and the ionosphere-thermosphere system. We study two main consequences of FACs in this system: the induced ground geomagnetic disturbances (GMDs), which arise as FACs close in the ionosphere, and the resultant Joule heating and perturbed thermospheric neutral winds as the energy transferred by FACs dissipates via their closure currents. We find, within data restrictions, no strong linear correlation between FAC and GMD magnitudes, instead suggesting solar wind parameters as a better indication of the location and strength of harmful ground GMDs. We probe the effect a neutral wind disparity between ground-based instrument and satellite measurements will have on the distribution and magnitude of wind-derived Joule heating, after using a model to show the winds should be equivalent. We suggest the cause of the disparity is due to uncertainties in the satellite wind derivation. Finally, we investigate small-scale FAC-driven Joule heating and electron precipitation as the causes of a satellite-measured cusp density enhancement and FPI-measured cusp and nightside auroral oval upwellings. We model an empirical heating source representative of soft and hard precipitation in these regions. Our simulations support a mechanism of soft precipitation and Joule heating in the cusp but are unable to reproduce the nightside upwelling. We suggest this is a storm-related anomaly, requiring an adjusted mechanism.
Supervisor: Not available Sponsor: Not available
Qualification Name: Thesis (Ph.D.) Qualification Level: Doctoral
EThOS ID: uk.bl.ethos.771813  DOI: Not available
Share: