The electric field response to the growth phase and expansion phase onset of a small isolated substorm

Lewis, R. V.; Freeman, M. P. ORCID: https://orcid.org/0000-0002-8653-8279; Rodger, A. S.; Reeves, G. D.; Milling, D. K.. 1997 The electric field response to the growth phase and expansion phase onset of a small isolated substorm. Annales Geophysicae, 15 (3). 289-299. 10.1007/s00585-997-0289-6

Full text not available from this repository. (Request a copy)

Abstract/Summary

We capitalise on the very large field of view of the Halley HF radar to provide a comprehensive description of the electric field response to the substorm growth phase and expansion phase onset of a relatively simple isolated substorm (|AL| < 250 nT) which occurred on 13 June 1988. The substorm phases are identified by their standard ground magnetic and spacecraft energetic particle signatures, which provide a framework for the radar measurements. The substorm is preceded by a prolonged period (> 12 h) of magnetic quiescence, such that prior to the start of the growth phase, the apparent latitudinal motion of the radar backscatter returns is consistent with the variation in latitude of the quiet-time auroral oval with magnetic local time. The growth phase is characterised by an increasing, superimposed equatorward motion of the equatorward edge of the radar backscatter as the auroral oval expands. Within this backscatter region, there is a poleward gradient in the Doppler spectral width, which we believe to correspond to latitudinal structure in auroral emissions and magnetospheric precipitation. During the growth phase the ionospheric convection is dominated by a relatively smooth largescale flow pattern consistent with the expanding DP2 (convection) auroral electrojets. Immediately prior to substorm onset the ionospheric convection observed by the radar in the midnight sector has a predominantly equatorward flow component. At substorm onset a dramatic change occurs and a poleward flow component prevails. The timing and location are quite remarkable. The timing of the flow change is within one minute of the dispersionless injection observed at geostationary orbit and the Pi2 magnetic signature on the ground. The location shows that this sudden change in flow is due to the effect of the upward field aligned current of the substorm current wedge imposed directly within the Halley radar field of view.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.1007/s00585-997-0289-6
Programmes:	BAS Programmes > Pre 2000 programme
ISSN:	1432-0576
Date made live:	26 Sep 2016 10:28 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/514578

Actions (login required)

View Item

Document Downloads

More statistics for this item...