The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

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

The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

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

Department of Physics

Research output: Contribution to conference › Abstract › peer-review

Abstract

Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.

Original language	English
Publication status	Published - 01 Dec 2008
Event	American Geophysical Union Fall Meeting - San Francisco, United States of America Duration: 15 Dec 2008 → 19 Dec 2008 Conference number: 2008

Conference

Conference	American Geophysical Union Fall Meeting
Abbreviated title	AGU
Country/Territory	United States of America
City	San Francisco
Period	15 Dec 2008 → 19 Dec 2008

Keywords

2102 Corotating streams
2154 Planetary bow shocks
2164 Solar wind plasma
2194 Instruments and techniques

Access to Document

http://adsabs.harvard.edu/abs/2008AGUFM.P13B1311W

Permanent link

Persistent link

Cite this

Whittaker, I. C., Grande, M., Guymer, G., Pintér, B., Barabash, S., Federov, A., Mazelle, C., Sauvaud, J., Lundin, R., Russell, C., Futaana, Y., Fränz, M., Zhang, T. L., Andersson, H., Brinkfeldt, K., Grigoriev, A., Holmströ M, M., Yamauchi, M., Asamura, K., ... Bochsler, P. (2008). The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.. Abstract from American Geophysical Union Fall Meeting, San Francisco, United States of America. http://adsabs.harvard.edu/abs/2008AGUFM.P13B1311W

@conference{6b66c823404c48a1910c42ee2124b49b,

title = "The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.",

abstract = "Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.",

keywords = "2102 Corotating streams, 2154 Planetary bow shocks, 2164 Solar wind plasma, 2194 Instruments and techniques",

author = "Whittaker, {I. C.} and M. Grande and G. Guymer and B. Pint{\'e}r and S. Barabash and A. Federov and C. Mazelle and J. Sauvaud and R. Lundin and C. Russell and Y. Futaana and M. Fr{\"a}nz and Zhang, {T. L.} and H. Andersson and K. Brinkfeldt and A. Grigoriev and {Holmstr{\"o} M}, M. and M. Yamauchi and K. Asamura and W. Baumjohann and H. Lammer and Coates, {A. J.} and Kataria, {D. O.} and Linder, {D. R.} and Curtis, {C. C.} and Hsieh, {K. C.} and Sandel, {B. R.} and H. Gunell and Koskinen, {H. E.} and E. Kallio and P. Riihel{\"a} and T. S{\"a}les and W. Schmidt and J. Kozyra and N. Krupp and J. Woch and J. Luhmann and S. McKenna-Lawlor and Thocaven, {J. J.} and S. Orsini and R. Cerulli-Irelli and M. Mura and M. Milillo and M. Maggi and E. Roelof and P. Brandt and K. Szego and Winningham, {J. D.} and Frahm, {R. A.} and J. Scherrer and J. Sharber and P. Wurz and P. Bochsler",

year = "2008",

month = dec,

day = "1",

language = "English",

note = "American Geophysical Union Fall Meeting, AGU ; Conference date: 15-12-2008 Through 19-12-2008",

}

Whittaker, IC, Grande, M, Guymer, G, Pintér, B, Barabash, S, Federov, A, Mazelle, C, Sauvaud, J, Lundin, R, Russell, C, Futaana, Y, Fränz, M, Zhang, TL, Andersson, H, Brinkfeldt, K, Grigoriev, A, Holmströ M, M, Yamauchi, M, Asamura, K, Baumjohann, W, Lammer, H, Coates, AJ, Kataria, DO, Linder, DR, Curtis, CC, Hsieh, KC, Sandel, BR, Gunell, H, Koskinen, HE, Kallio, E, Riihelä, P, Säles, T, Schmidt, W, Kozyra, J, Krupp, N, Woch, J, Luhmann, J, McKenna-Lawlor, S, Thocaven, JJ, Orsini, S, Cerulli-Irelli, R, Mura, M, Milillo, M, Maggi, M, Roelof, E, Brandt, P, Szego, K, Winningham, JD, Frahm, RA, Scherrer, J, Sharber, J, Wurz, P & Bochsler, P 2008, 'The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.', American Geophysical Union Fall Meeting, San Francisco, United States of America, 15 Dec 2008 - 19 Dec 2008. <http://adsabs.harvard.edu/abs/2008AGUFM.P13B1311W>

TY - CONF

T1 - The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

AU - Whittaker, I. C.

AU - Grande, M.

AU - Guymer, G.

AU - Pintér, B.

AU - Barabash, S.

AU - Federov, A.

AU - Mazelle, C.

AU - Sauvaud, J.

AU - Lundin, R.

AU - Russell, C.

AU - Futaana, Y.

AU - Fränz, M.

AU - Zhang, T. L.

AU - Andersson, H.

AU - Brinkfeldt, K.

AU - Grigoriev, A.

AU - Holmströ M, M.

AU - Yamauchi, M.

AU - Asamura, K.

AU - Baumjohann, W.

AU - Lammer, H.

AU - Coates, A. J.

AU - Kataria, D. O.

AU - Linder, D. R.

AU - Curtis, C. C.

AU - Hsieh, K. C.

AU - Sandel, B. R.

AU - Gunell, H.

AU - Koskinen, H. E.

AU - Kallio, E.

AU - Riihelä, P.

AU - Säles, T.

AU - Schmidt, W.

AU - Kozyra, J.

AU - Krupp, N.

AU - Woch, J.

AU - Luhmann, J.

AU - McKenna-Lawlor, S.

AU - Thocaven, J. J.

AU - Orsini, S.

AU - Cerulli-Irelli, R.

AU - Mura, M.

AU - Milillo, M.

AU - Maggi, M.

AU - Roelof, E.

AU - Brandt, P.

AU - Szego, K.

AU - Winningham, J. D.

AU - Frahm, R. A.

AU - Scherrer, J.

AU - Sharber, J.

AU - Wurz, P.

AU - Bochsler, P.

N1 - Conference code: 2008

PY - 2008/12/1

Y1 - 2008/12/1

N2 - Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.

AB - Using the ASPERA-4 instrument onboard Venus Express the change in the atmospheric boundary layers are investigated. Using the instrument when it is in the apoapsis period of the polar orbit allows pure Solar Wind measurements to be taken. Composition ratios are determined thus identifying periods of fast and slow solar wind. This is then applied to ion maps of the Venusian atmosphere to determine the response after noise calibration methods. The Species reactions to the differing Solar Wind are also used to investigate the inner boundary movements.

KW - 2102 Corotating streams

KW - 2154 Planetary bow shocks

KW - 2164 Solar wind plasma

KW - 2194 Instruments and techniques

M3 - Abstract

T2 - American Geophysical Union Fall Meeting

Y2 - 15 December 2008 through 19 December 2008

ER -

The Effect Of Fast And Slow Solar Wind On The Venusian Upper Atmosphere.

Abstract

Conference

Keywords

Access to Document

Permanent link

Fingerprint

Cite this