1999
DOI: 10.1029/1998gl900242
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Footprints of lobe reconnection observed in ionospheric electron density under steady northward IMF

Abstract: Abstract. The paper focuses on ionospheric signatures of lobe reconnection near magnetic noon under steady northward IMF. Enhanced Type 2 aurora observed by a meridian scanning photometer and reverse ion energy dispersion measured during a DMSP satellite pass provide evidence for the reconnection. Tomographic imaging of the spatial plasma distribution reveals key footprints of the processes, including the location of the adiaroic boundary separating the lobe cells from the closed LLBL precipitation, the disper… Show more

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Cited by 6 publications
(7 citation statements)
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“…There is a coexistence of type 1 and type 2 auroral forms for clock angles between 45°and 90°. Footprint signatures of reconnection processes in the spatial distribution of the ionospheric plasma density were reported by Walker et al (1998) and Pryse et al (1999) for Bz negative and positive respectively. The former study identi®ed a density enhancement co-located with type 1 aurora, with a steep density gradient on its equatorward side.…”
Section: Introductionmentioning
confidence: 99%
“…There is a coexistence of type 1 and type 2 auroral forms for clock angles between 45°and 90°. Footprint signatures of reconnection processes in the spatial distribution of the ionospheric plasma density were reported by Walker et al (1998) and Pryse et al (1999) for Bz negative and positive respectively. The former study identi®ed a density enhancement co-located with type 1 aurora, with a steep density gradient on its equatorward side.…”
Section: Introductionmentioning
confidence: 99%
“…It is clear that tomographic imaging opens up the possibility of identifying characteristic features in the plasma distribution, like the depleted troughs, enhanced blobs and ionization tongues, of the complex structures that form the polar ionosphere. Boundaries between different plasma regimes in flux tubes linked to vastly separate regions of space can be identified in tomographic images [e.g., Walker et al , 1998; Pryse et al , 1999] so that use of observations from several chains of stations opens up the possibility of relating boundaries seen in the different geomagnetic sectors at the same time. A later study concerns the important topic of the structure of the polar ionosphere under northward IMF [ Middleton et al , 2005].…”
Section: Discussionmentioning
confidence: 99%
“…Several papers have addressed such issues, including two that illustrate the signatures in the dayside cusp ionosphere of the reconnection processes that link the Interplanetary Magnetic Field (IMF) carried by the solar wind to the geomagnetic field. Walker et al (1998) used radio tomography to image features resulting from reconnection near the equatorial plane when the IMF was southwards, while Pryse et al (1999) discussed structures linked to lobe reconnection under northwards IMF.…”
Section: Tomography and Space Weathermentioning
confidence: 99%