Relation between discrete auroral forms and magnetic field disturbances

Autor: Lanchester, B. S.

Externí odkaz: http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.356061

Using spectral characteristics to interpret auroral imaging in the 731.9 nm O+ line

Autor: Dahlgren, H., Nickolay Ivchenko, Lanchester, B. S., Sullivan, J., Whiter, D., Marklund, G., Strømme, A.

Publikováno v: Scopus-Elsevier

Simultaneous observations were made of dynamic aurora during substorm activity on 26 January 2006 with three high spatial and temporal resolution instruments: the ASK (Auroral Structure and Kinetics) instrument, SIF (Spectrographic Imaging Facility)

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::574369160c25f49e245d7a3b0c5e31e3
https://www.ann-geophys.net/26/1905/2008/

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.

Auroral Small-and Meso-Scale Structures, Origin and Function

Autor: Frey, H. U., Amm, O., Chaston, C. C., Fu, S., Haerendel, G., Juusola, L., Karlsson, R., Lanchester, B. S., Nakamura, R., Ostgaard, N., Sakanoi, T., Seran, Elena, Whiter, D.

Publikováno v: American Geophysical Union Fall Meeting 2009
American Geophysical Union Fall Meeting 2009, Dec 2009, San Francisco California, United States. pp.abstract id.SM52B-05

International audience; Discrete auroral arcs regularly display small- and meso-scale distortions that can appear suddenly and move with speeds that are not related to plasma speeds in the ionosphere but rather represent properties of the acceleratio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______2417::7eef8f7688c1d7c5031a2df213e64f69
https://hal.science/hal-04113486

Modeling the observed proton aurora and ionospheric convection responses to changes in the IMF clock angle: 2. Persistence of ionospheric convection

Autor: Lockwood, Mike, Lanchester, B. S., Morley, S. K., Throp, K., Milan, S. E., Lester, M., Frey, H. U.

We apply a numerical model of time-dependent ionospheric convection to two directly driven reconnection pulses during a 15-min interval of southward IMF on 26 November 2000. The model requires an input magnetopause reconnection rate variation, which

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::ed4554094701ebfc1eb8abb1fef3a283
https://centaur.reading.ac.uk/38581/1/231_Lockwood_2003JA010307f.pdf