Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/7903
Title: Multi-instrument observations of the ionospheric counterpart of a bursty bulk flow in the near-Earth plasma sheet
Authors: Grocott, Adrian
Yeoman, Tim K.
Nakamura, R.
Cowley, S. W. H.
Frey, H. U.
Rème, H.
Klecker, B.
First Published: 2-Apr-2004
Publisher: European Geosciences Union (EGU)
Citation: Annales Geophysicae, 2004, 22 (4), pp. 1061-1075.
Abstract: On 07 September 2001 the Cluster spacecraft observed a "bursty bulk flow" event in the near-Earth central plasma sheet. This paper presents a detailed study of the coincident ground-based observations and attempts to place them within a simple physical framework. The event in question occurs at ~22:30 UT, some 10min after a southward turning of the IMF. IMAGE and SAMNET magnetometer measurements of the ground magnetic field reveal perturbations of a few tens of nT and small amplitude Pi2 pulsations. CUTLASS radar observations of ionospheric plasma convection show enhanced flows out of the polar cap near midnight, accompanied by an elevated transpolar voltage. Optical data from the IMAGE satellite also show that there is a transient, localised ~1 kR brightening in the UV aurora. These observations are consistent with the earthward transport of plasma in the tail, but also indicate the absence of a typical "large-scale" substorm current wedge. An analysis of the field-aligned current system implied by the radar measurements does suggest the existence of a small-scale current "wedgelet", but one which lacks the global scale and high conductivities observed during substorm expansions.
DOI Link: 10.5194/angeo-22-1061-2004
ISSN: 0992-7689
Links: http://www.ann-geophys.net/22/1061/2004/angeo-22-1061-2004.html
http://hdl.handle.net/2381/7903
Type: Article
Rights: This paper was published as Annales Geophysicae, 2004, 22 (4), pp. 1061-1075. It is also available from the publisher's website at http://www.ann-geophys.net/22/1061/2004/angeo-22-1061-2004.html © Author(s) 2004. This work is distributed under the Creative Commons Attribution 3.0 License.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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