The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission

E. Kallio; T. L. Zhang; S. Barabash; R. Jarvinen; I. Sillanpää; P. Janhunen; A. Fedorov; A. J. Sauvaud; C. Mazelle; J. J. Thocaven; H. Gunell; H. Andersson; A. Grigoriev; K. Brinkfeldt; Y. Futaana; M. Holmström; R. Lundin; M. Yamauchi; K. Asamura; W. Baumjohann; H. Lammer; A. J. Coates; D. R. Linder; D. O. Kataria; C. C. Curtis; K. C. Hsieh; B. R. Sandel; M. Grande; H. E. J. Koskinen; T. Säles; W. Schmidt; P. Riihelä; J. Kozyra; N. Krupp; J. Woch; J. G. Luhmann; S. McKenna-Lawlor; S. Orsini; R. Cerulli-Irelli; A. Mura; A. Milillo; M. Maggi; E. Roelof; P. Brandt; C. T. Russell; K. Szego; J. D. Winningham; R. A. Frahm; J. R. Scherrer; J. R. Sharber; P. Wurz; P. Bochsler

The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission

E. Kallio, T. L. Zhang, S. Barabash, R. Jarvinen, I. Sillanpää, P. Janhunen, A. Fedorov, A. J. Sauvaud, C. Mazelle, J. J. Thocaven, H. Gunell, H. Andersson, A. Grigoriev, K. Brinkfeldt, Y. Futaana, M. Holmström, R. Lundin, M. Yamauchi, K. Asamura, W. BaumjohannH. Lammer, A. J. Coates, D. R. Linder, D. O. Kataria, C. C. Curtis, K. C. Hsieh, B. R. Sandel, M. Grande, H. E. J. Koskinen, T. Säles, W. Schmidt, P. Riihelä, J. Kozyra, N. Krupp, J. Woch, J. G. Luhmann, S. McKenna-Lawlor, S. Orsini, R. Cerulli-Irelli, A. Mura, A. Milillo, M. Maggi, E. Roelof, P. Brandt, C. T. Russell, K. Szego, J. D. Winningham, R. A. Frahm, J. R. Scherrer, J. R. Sharber, P. Wurz, P. Bochsler

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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.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	796-801
Nifer y tudalennau	6
Cyfnodolyn	Planetary and Space Science
Cyfrol	56
Rhif cyhoeddi	6
Statws	Cyhoeddwyd - 31 Mai 2008

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http://hdl.handle.net/2160/8593

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Kallio, E., Zhang, T. L., Barabash, S., Jarvinen, R., Sillanpää, I., Janhunen, P., Fedorov, A., Sauvaud, A. J., Mazelle, C., Thocaven, J. J., Gunell, H., Andersson, H., Grigoriev, A., Brinkfeldt, K., Futaana, Y., Holmström, M., Lundin, R., Yamauchi, M., Asamura, K., ... Bochsler, P. (2008). The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission. Planetary and Space Science, 56(6), 796-801.

@article{d11e545fcd0a4733891d8225897c94f2,

title = "The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission",

abstract = "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.",

author = "E. Kallio and Zhang, {T. L.} and S. Barabash and R. Jarvinen and I. Sillanp{\"a}{\"a} and P. Janhunen and A. Fedorov and Sauvaud, {A. J.} and C. Mazelle and Thocaven, {J. J.} and H. Gunell and H. Andersson and A. Grigoriev and K. Brinkfeldt and Y. Futaana and M. Holmstr{\"o}m and R. Lundin and M. Yamauchi and K. Asamura and W. Baumjohann and H. Lammer and Coates, {A. J.} and Linder, {D. R.} and Kataria, {D. O.} and Curtis, {C. C.} and Hsieh, {K. C.} and Sandel, {B. R.} and M. Grande and Koskinen, {H. E. J.} and T. S{\"a}les and W. Schmidt and P. Riihel{\"a} and J. Kozyra and N. Krupp and J. Woch and Luhmann, {J. G.} and S. McKenna-Lawlor and S. Orsini and R. Cerulli-Irelli and A. Mura and A. Milillo and M. Maggi and E. Roelof and P. Brandt and Russell, {C. T.} and K. Szego and Winningham, {J. D.} and Frahm, {R. A.} and Scherrer, {J. R.} and Sharber, {J. R.} and P. Wurz and P. Bochsler",

note = "specialissue: Mars Express/Venus Express ",

year = "2008",

month = may,

day = "31",

language = "English",

volume = "56",

pages = "796--801",

journal = "Planetary and Space Science",

issn = "0032-0633",

publisher = "Elsevier",

number = "6",

}

Kallio, E, Zhang, TL, Barabash, S, Jarvinen, R, Sillanpää, I, Janhunen, P, Fedorov, A, Sauvaud, AJ, Mazelle, C, Thocaven, JJ, Gunell, H, Andersson, H, Grigoriev, A, Brinkfeldt, K, Futaana, Y, Holmström, 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, Säles, T, Schmidt, W, Riihelä, 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, 'The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission', Planetary and Space Science, cyfrol. 56, rhif 6, tt. 796-801.

TY - JOUR

T1 - The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission

AU - Kallio, E.

AU - Zhang, T. L.

AU - Barabash, S.

AU - Jarvinen, R.

AU - Sillanpää, I.

AU - Janhunen, P.

AU - Fedorov, A.

AU - Sauvaud, A. J.

AU - Mazelle, C.

AU - Thocaven, J. J.

AU - Gunell, H.

AU - Andersson, H.

AU - Grigoriev, A.

AU - Brinkfeldt, K.

AU - Futaana, Y.

AU - Holmström, M.

AU - Lundin, R.

AU - Yamauchi, M.

AU - Asamura, K.

AU - Baumjohann, W.

AU - Lammer, H.

AU - Coates, A. J.

AU - Linder, D. R.

AU - Kataria, D. O.

AU - Curtis, C. C.

AU - Hsieh, K. C.

AU - Sandel, B. R.

AU - Grande, M.

AU - Koskinen, H. E. J.

AU - Säles, T.

AU - Schmidt, W.

AU - Riihelä, P.

AU - Kozyra, J.

AU - Krupp, N.

AU - Woch, J.

AU - Luhmann, J. G.

AU - McKenna-Lawlor, S.

AU - Orsini, S.

AU - Cerulli-Irelli, R.

AU - Mura, A.

AU - Milillo, A.

AU - Maggi, M.

AU - Roelof, E.

AU - Brandt, P.

AU - Russell, C. T.

AU - Szego, K.

AU - Winningham, J. D.

AU - Frahm, R. A.

AU - Scherrer, J. R.

AU - Sharber, J. R.

AU - Wurz, P.

AU - Bochsler, P.

N1 - specialissue: Mars Express/Venus Express

PY - 2008/5/31

Y1 - 2008/5/31

N2 - 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.

AB - 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.

UR - http://hdl.handle.net/2160/8593

M3 - Special Issue

SN - 0032-0633

VL - 56

SP - 796

EP - 801

JO - Planetary and Space Science

JF - Planetary and Space Science

IS - 6

ER -

The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission

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