Home > Research > Publications & Outputs > High-time resolution radar observations of high...
View graph of relations

High-time resolution radar observations of high-latitude flows during an isolated substorm

Research output: Contribution to conference - Without ISBN/ISSN Otherpeer-review

Published

Standard

High-time resolution radar observations of high-latitude flows during an isolated substorm. / Wild, J.A.; Yeoman, T.K.; Davies, J.A.
2000. Proceedings of the SuperDARN Workshop.

Research output: Contribution to conference - Without ISBN/ISSN Otherpeer-review

Harvard

Wild, JA, Yeoman, TK & Davies, JA 2000, 'High-time resolution radar observations of high-latitude flows during an isolated substorm', Proceedings of the SuperDARN Workshop, 1/01/00.

APA

Wild, J. A., Yeoman, T. K., & Davies, J. A. (2000). High-time resolution radar observations of high-latitude flows during an isolated substorm. Proceedings of the SuperDARN Workshop.

Vancouver

Wild JA, Yeoman TK, Davies JA. High-time resolution radar observations of high-latitude flows during an isolated substorm. 2000. Proceedings of the SuperDARN Workshop.

Author

Wild, J.A. ; Yeoman, T.K. ; Davies, J.A. / High-time resolution radar observations of high-latitude flows during an isolated substorm. Proceedings of the SuperDARN Workshop.

Bibtex

@conference{f7feb7f39f874bab953c7ab8cc68c979,
title = "High-time resolution radar observations of high-latitude flows during an isolated substorm",
abstract = "High-time resolution CUTLASS observations and ground-based magnetometers have been employed to study the occurrence of vortical flow structures propagating through the high-latitude ionosphere during magnetospheric substorms. Fast-moving flow vortices (~800 m/s) associated with Hall currents flowing around upward directed feld-aligned currents are frequently observed propagating at high speed (~1 km/s) azimuthally away from the region of the ionosphere associated with the location of the substorm expansion phase onset. Furthermore, a statistical analysis drawn from over 1000 h of high-time resolution, nightside radar data has enabled the characterisation of the bulk properties of these vortical flow systems. Their occurrence with respect to substorm phase has been investigated and a possible generation mechanism has been suggested.",
author = "J.A. Wild and T.K. Yeoman and J.A. Davies",
year = "2000",
language = "English",
note = "Proceedings of the SuperDARN Workshop ; Conference date: 01-01-1900",

}

RIS

TY - CONF

T1 - High-time resolution radar observations of high-latitude flows during an isolated substorm

AU - Wild, J.A.

AU - Yeoman, T.K.

AU - Davies, J.A.

PY - 2000

Y1 - 2000

N2 - High-time resolution CUTLASS observations and ground-based magnetometers have been employed to study the occurrence of vortical flow structures propagating through the high-latitude ionosphere during magnetospheric substorms. Fast-moving flow vortices (~800 m/s) associated with Hall currents flowing around upward directed feld-aligned currents are frequently observed propagating at high speed (~1 km/s) azimuthally away from the region of the ionosphere associated with the location of the substorm expansion phase onset. Furthermore, a statistical analysis drawn from over 1000 h of high-time resolution, nightside radar data has enabled the characterisation of the bulk properties of these vortical flow systems. Their occurrence with respect to substorm phase has been investigated and a possible generation mechanism has been suggested.

AB - High-time resolution CUTLASS observations and ground-based magnetometers have been employed to study the occurrence of vortical flow structures propagating through the high-latitude ionosphere during magnetospheric substorms. Fast-moving flow vortices (~800 m/s) associated with Hall currents flowing around upward directed feld-aligned currents are frequently observed propagating at high speed (~1 km/s) azimuthally away from the region of the ionosphere associated with the location of the substorm expansion phase onset. Furthermore, a statistical analysis drawn from over 1000 h of high-time resolution, nightside radar data has enabled the characterisation of the bulk properties of these vortical flow systems. Their occurrence with respect to substorm phase has been investigated and a possible generation mechanism has been suggested.

M3 - Other

T2 - Proceedings of the SuperDARN Workshop

Y2 - 1 January 1900

ER -