The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed and compared with predictions of a global model. It is shown that in the orbit studied, the plasma and magnetic field observations obtained near the North Pole under solar minimum conditions were qual...
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PERGAMON-ELSEVIER SCIENCE LTD
2008
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Online Access: | http://discovery.ucl.ac.uk/114085/ |
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ftucl:oai:eprints.ucl.ac.uk.OAI2:114085 2023-05-15T17:39:49+02:00 The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission Kallio, E Zhang, TL Barabash, S Jarvinen, R Sillanpaa, I Janhunen, P Fedorov, A Sauvaud, JA Mazelle, C Thocaven, JJ Gunell, H Andersson, H Grigoriev, A Brinkfeldt, K Futaana, Y Holmstrom, M Lundin, R Yamauchi, M Asamura, K Baumjohann, W Lammer, H Coates, AJ Linder, DR Kataria, DO Curtis, CC Hsieh, KC Sandel, BR Grande, M Koskinen, HEJ Sales, T Schmidt, W Riihela, P Kozyra, J Krupp, N Woch, J Luhmann, JG McKenna-Lawlor, S Orsini, S Cerulli-Irelli, R Mura, A Milillo, A Maggi, M Roelof, E Brandt, P Russell, CT Szego, K Winningham, JD Frahm, RA Scherrer, JR Sharber, JR Wurz, P Bochsler, P 2008-05 http://discovery.ucl.ac.uk/114085/ unknown PERGAMON-ELSEVIER SCIENCE LTD PLANET SPACE SCI , 56 (6) 796 - 801. (2008) Venus Venus-solar wind interaction planetary magnetospheres solar wind numerical modelling Article 2008 ftucl 2016-01-15T02:50:58Z Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed and compared with predictions of a global model. It is shown that in the orbit studied, the plasma and magnetic field observations obtained near the North Pole under solar minimum conditions were qualitatively and, in many cases also, quantitatively in agreement with the general picture obtained using a global numerical quasi-neutral hybrid model of the solar wind interaction (HYB-Venus). In instances where the orbit of Venus Express crossed a boundary referred to as the magnetic pileup boundary (MPB), field line tracing supports the suggestion that the MPB separates the region that is magnetically connected to the fluctuating magnetosheath field from a region that is magnetically connected to the induced magnetotail lobes. (c) 2007 Elsevier Ltd. All rights reserved. Article in Journal/Newspaper North Pole University College London: UCL Discovery North Pole Venus ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
institution |
Open Polar |
collection |
University College London: UCL Discovery |
op_collection_id |
ftucl |
language |
unknown |
topic |
Venus Venus-solar wind interaction planetary magnetospheres solar wind numerical modelling |
spellingShingle |
Venus Venus-solar wind interaction planetary magnetospheres solar wind numerical modelling Kallio, E Zhang, TL Barabash, S Jarvinen, R Sillanpaa, I Janhunen, P Fedorov, A Sauvaud, JA Mazelle, C Thocaven, JJ Gunell, H Andersson, H Grigoriev, A Brinkfeldt, K Futaana, Y Holmstrom, M Lundin, R Yamauchi, M Asamura, K Baumjohann, W Lammer, H Coates, AJ Linder, DR Kataria, DO Curtis, CC Hsieh, KC Sandel, BR Grande, M Koskinen, HEJ Sales, T Schmidt, W Riihela, P Kozyra, J Krupp, N Woch, J Luhmann, JG McKenna-Lawlor, S Orsini, S Cerulli-Irelli, R Mura, A Milillo, A Maggi, M Roelof, E Brandt, P Russell, CT Szego, K Winningham, JD Frahm, RA Scherrer, JR Sharber, JR Wurz, P Bochsler, P The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
topic_facet |
Venus Venus-solar wind interaction planetary magnetospheres solar wind numerical modelling |
description |
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed and compared with predictions of a global model. It is shown that in the orbit studied, the plasma and magnetic field observations obtained near the North Pole under solar minimum conditions were qualitatively and, in many cases also, quantitatively in agreement with the general picture obtained using a global numerical quasi-neutral hybrid model of the solar wind interaction (HYB-Venus). In instances where the orbit of Venus Express crossed a boundary referred to as the magnetic pileup boundary (MPB), field line tracing supports the suggestion that the MPB separates the region that is magnetically connected to the fluctuating magnetosheath field from a region that is magnetically connected to the induced magnetotail lobes. (c) 2007 Elsevier Ltd. All rights reserved. |
format |
Article in Journal/Newspaper |
author |
Kallio, E Zhang, TL Barabash, S Jarvinen, R Sillanpaa, I Janhunen, P Fedorov, A Sauvaud, JA Mazelle, C Thocaven, JJ Gunell, H Andersson, H Grigoriev, A Brinkfeldt, K Futaana, Y Holmstrom, M Lundin, R Yamauchi, M Asamura, K Baumjohann, W Lammer, H Coates, AJ Linder, DR Kataria, DO Curtis, CC Hsieh, KC Sandel, BR Grande, M Koskinen, HEJ Sales, T Schmidt, W Riihela, P Kozyra, J Krupp, N Woch, J Luhmann, JG McKenna-Lawlor, S Orsini, S Cerulli-Irelli, R Mura, A Milillo, A Maggi, M Roelof, E Brandt, P Russell, CT Szego, K Winningham, JD Frahm, RA Scherrer, JR Sharber, JR Wurz, P Bochsler, P |
author_facet |
Kallio, E Zhang, TL Barabash, S Jarvinen, R Sillanpaa, I Janhunen, P Fedorov, A Sauvaud, JA Mazelle, C Thocaven, JJ Gunell, H Andersson, H Grigoriev, A Brinkfeldt, K Futaana, Y Holmstrom, M Lundin, R Yamauchi, M Asamura, K Baumjohann, W Lammer, H Coates, AJ Linder, DR Kataria, DO Curtis, CC Hsieh, KC Sandel, BR Grande, M Koskinen, HEJ Sales, T Schmidt, W Riihela, P Kozyra, J Krupp, N Woch, J Luhmann, JG McKenna-Lawlor, S Orsini, S Cerulli-Irelli, R Mura, A Milillo, A Maggi, M Roelof, E Brandt, P Russell, CT Szego, K Winningham, JD Frahm, RA Scherrer, JR Sharber, JR Wurz, P Bochsler, P |
author_sort |
Kallio, E |
title |
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
title_short |
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
title_full |
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
title_fullStr |
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
title_full_unstemmed |
The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission |
title_sort |
venusian induced magnetosphere: a case study of plasma and magnetic field measurements on the venus express mission |
publisher |
PERGAMON-ELSEVIER SCIENCE LTD |
publishDate |
2008 |
url |
http://discovery.ucl.ac.uk/114085/ |
long_lat |
ENVELOPE(-57.842,-57.842,-61.925,-61.925) |
geographic |
North Pole Venus |
geographic_facet |
North Pole Venus |
genre |
North Pole |
genre_facet |
North Pole |
op_source |
PLANET SPACE SCI , 56 (6) 796 - 801. (2008) |
_version_ |
1766140591487320064 |