Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36461
Title: Substorm related changes in precipitation in the dayside auroral zone – a multi instrument case study
Authors: Kavanagh, A. J.
Honary, F.
McCrea, I. W.
Donovan, E.
Woodfield, E. E.
Manninen, J.
Anderson, P. C.
First Published: 30-Sep-2002
Publisher: European Geosciences Union (EGU), Copernicus Publications, Springer Verlag (Germany)
Citation: Annales Geophysicae, 20, 1321-1334, 2002
Abstract: A period (08:10–14:40 MLT, 11 February 1997) of enhanced electron density in the D- and E-regions is investigated using EISCAT, IRIS and other complementary instruments. The precipitation is determined to be due to substorm processes occurring close to magnetic midnight. Energetic electrons drift eastward after substorm injection and precipitate in the morning sector. The precipitation is triggered by small pulses in the solar wind pressure, which drive wave particle interactions. The characteristic energy of precipitation is inferred from drift timing on different L-shells and apparently verified by EISCAT measurements. The IMF influence on the precipitation in the auroral zone is also briefly discussed. A large change in the precipitation spectrum is attributed to increased numbers of ions and much reduced electron fluxes. These are detected by a close passing DMSP satellite. The possibility that these ions are from the low latitude boundary layer (LLBL) is discussed with reference to structured narrow band Pc1 waves observed by a search coil magnetometer, co-located with IRIS. The intensity of the waves grows with increased distance equatorward of the cusp position (determined by both satellite and HF radar), contrary to expectations if the precipitation is linked to the LLBL. It is suggested that the ion precipitation is, instead, due to the recovery phase of a small geomagnetic storm, following on from very active conditions. The movement of absorption in the later stages of the event is compared with observations of the ionospheric convection velocities. A good agreement is found to exist in this time interval suggesting that E × B drift has become the dominant drift mechanism over the gradient-curvature drift separation of the moving absorption patches observed at the beginning of the morning precipitation event.
DOI Link: 10.5194/angeo-20-1321-2002
ISSN: 0992-7689
eISSN: 1432-0576
Links: http://www.ann-geophys.net/20/1321/2002/
http://hdl.handle.net/2381/36461
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © Author(s) 2002. This work is distributed under the Creative Commons Attribution 3.0 License.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
angeo-20-1321-2002.pdfPublisher version554.45 kBAdobe PDFView/Open


Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.