The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission

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

doi:10.1016/j.pss.2007.01.014

The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission

S. Barabash^*, J. A. Sauvaud, H. Gunell, H. Andersson, A. Grigoriev, K. Brinkfeldt, M. Holmström, R. Lundin, M. Yamauchi, K. Asamura, W. Baumjohann, T. L. Zhang, A. J. Coates, D. R. Linder, D. O. Kataria, C. C. Curtis, K. C. Hsieh, B. R. Sandel, A. Fedorov, C. MazelleJ. J. Thocaven, M. Grande, Hannu E.J. Koskinen, E. Kallio, T. Säles, P. Riihela, J. Kozyra, N. Krupp, J. Woch, J. Luhmann, S. McKenna-Lawlor, S. Orsini, R. Cerulli-Irelli, M. Mura, M. Milillo, M. Maggi, E. Roelof, P. Brandt, C. T. Russell, K. Szego, J. D. Winningham, R. A. Frahm, J. Scherrer, J. R. Sharber, P. Wurz, P. Bochsler

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The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) experiment is to study the solar wind-atmosphere interaction and characterise the plasma and neutral gas environment in the near-Venus space through energetic neutral atom (ENA) imaging and local charged particle measurements. The studies to be performed address the fundamental question: How strongly do the interplanetary plasma and electromagnetic fields affect the Venusian atmosphere? The ASPERA-4 instrument comprises four sensors; two ENA sensors, electron and ion spectrometers. The neutral particle imager (NPI) provides measurements of the integral ENA flux (0.1-60 keV) with no mass and energy resolution but relatively high angular resolution. The neutral particle detector (NPD) provides measurements of the ENA flux, resolving velocity (0.1-10 keV) and mass (H and O) with a coarse angular resolution. The electron spectrometer (ELS) is a standard top-hat electrostatic analyser in a very compact design. These three sensors are located on a scanning platform providing a 4 π coverage. The instrument also contains an ion mass composition sensor, IMA (ion mass analyser). Mechanically, IMA is a separate unit electrically connected with the ASPERA-4 main unit. IMA provides ion measurements in the energy range 0.01-36 keV/q for the main ion components H⁺, He⁺⁺, He⁺, and the ion group with M / q 20 - 80 amu / q.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	1772-1792
Nifer y tudalennau	21
Cyfnodolyn	Planetary and Space Science
Cyfrol	55
Rhif cyhoeddi	12
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1016/j.pss.2007.01.014
Statws	Cyhoeddwyd - Hyd 2007

Mynediad at Ddogfen

10.1016/j.pss.2007.01.014

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Dolen i’r cyhoeddiad yn Scopus

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Barabash, S., Sauvaud, J. A., Gunell, H., Andersson, H., Grigoriev, A., Brinkfeldt, K., Holmström, M., Lundin, R., Yamauchi, M., Asamura, K., Baumjohann, W., Zhang, T. L., Coates, A. J., Linder, D. R., Kataria, D. O., Curtis, C. C., Hsieh, K. C., Sandel, B. R., Fedorov, A., ... Bochsler, P. (2007). The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission. Planetary and Space Science, 55(12), 1772-1792. https://doi.org/10.1016/j.pss.2007.01.014

@article{27bdad9671b0417199bcbd30ed18a84d,

title = "The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission",

abstract = "The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) experiment is to study the solar wind-atmosphere interaction and characterise the plasma and neutral gas environment in the near-Venus space through energetic neutral atom (ENA) imaging and local charged particle measurements. The studies to be performed address the fundamental question: How strongly do the interplanetary plasma and electromagnetic fields affect the Venusian atmosphere? The ASPERA-4 instrument comprises four sensors; two ENA sensors, electron and ion spectrometers. The neutral particle imager (NPI) provides measurements of the integral ENA flux (0.1-60 keV) with no mass and energy resolution but relatively high angular resolution. The neutral particle detector (NPD) provides measurements of the ENA flux, resolving velocity (0.1-10 keV) and mass (H and O) with a coarse angular resolution. The electron spectrometer (ELS) is a standard top-hat electrostatic analyser in a very compact design. These three sensors are located on a scanning platform providing a 4 π coverage. The instrument also contains an ion mass composition sensor, IMA (ion mass analyser). Mechanically, IMA is a separate unit electrically connected with the ASPERA-4 main unit. IMA provides ion measurements in the energy range 0.01-36 keV/q for the main ion components H+, He++, He+, and the ion group with M / q 20 - 80 amu / q.",

keywords = "Energetic neutral atom imagers, Ion and electron analysers, Space instrumentation, Venus",

author = "S. Barabash and Sauvaud, {J. A.} and H. Gunell and H. Andersson and A. Grigoriev and K. Brinkfeldt and M. Holmstr{\"o}m and R. Lundin and M. Yamauchi and K. Asamura and W. Baumjohann and Zhang, {T. L.} 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 A. Fedorov and C. Mazelle and Thocaven, {J. J.} and M. Grande and Koskinen, {Hannu E.J.} and E. Kallio and T. S{\"a}les and P. Riihela and J. Kozyra and N. Krupp and J. Woch and J. Luhmann and S. McKenna-Lawlor and S. Orsini and R. Cerulli-Irelli and M. Mura and M. 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 J. Scherrer and Sharber, {J. R.} and P. Wurz and P. Bochsler",

year = "2007",

month = oct,

doi = "10.1016/j.pss.2007.01.014",

language = "English",

volume = "55",

pages = "1772--1792",

journal = "Planetary and Space Science",

issn = "0032-0633",

publisher = "Elsevier",

number = "12",

}

Barabash, S, Sauvaud, JA, Gunell, H, Andersson, H, Grigoriev, A, Brinkfeldt, K, Holmström, M, Lundin, R, Yamauchi, M, Asamura, K, Baumjohann, W, Zhang, TL, Coates, AJ, Linder, DR, Kataria, DO, Curtis, CC, Hsieh, KC, Sandel, BR, Fedorov, A, Mazelle, C, Thocaven, JJ, Grande, M, Koskinen, HEJ, Kallio, E, Säles, T, Riihela, P, Kozyra, J, Krupp, N, Woch, J, Luhmann, J, McKenna-Lawlor, S, Orsini, S, Cerulli-Irelli, R, Mura, M, Milillo, M, Maggi, M, Roelof, E, Brandt, P, Russell, CT, Szego, K, Winningham, JD, Frahm, RA, Scherrer, J, Sharber, JR, Wurz, P & Bochsler, P 2007, 'The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission', Planetary and Space Science, cyfrol. 55, rhif 12, tt. 1772-1792. https://doi.org/10.1016/j.pss.2007.01.014

TY - JOUR

T1 - The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission

AU - Barabash, S.

AU - Sauvaud, J. A.

AU - Gunell, H.

AU - Andersson, H.

AU - Grigoriev, A.

AU - Brinkfeldt, K.

AU - Holmström, M.

AU - Lundin, R.

AU - Yamauchi, M.

AU - Asamura, K.

AU - Baumjohann, W.

AU - Zhang, T. L.

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 - Fedorov, A.

AU - Mazelle, C.

AU - Thocaven, J. J.

AU - Grande, M.

AU - Koskinen, Hannu E.J.

AU - Kallio, E.

AU - Säles, T.

AU - Riihela, P.

AU - Kozyra, J.

AU - Krupp, N.

AU - Woch, J.

AU - Luhmann, J.

AU - McKenna-Lawlor, S.

AU - Orsini, S.

AU - Cerulli-Irelli, R.

AU - Mura, M.

AU - Milillo, M.

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.

AU - Sharber, J. R.

AU - Wurz, P.

AU - Bochsler, P.

PY - 2007/10

Y1 - 2007/10

N2 - The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) experiment is to study the solar wind-atmosphere interaction and characterise the plasma and neutral gas environment in the near-Venus space through energetic neutral atom (ENA) imaging and local charged particle measurements. The studies to be performed address the fundamental question: How strongly do the interplanetary plasma and electromagnetic fields affect the Venusian atmosphere? The ASPERA-4 instrument comprises four sensors; two ENA sensors, electron and ion spectrometers. The neutral particle imager (NPI) provides measurements of the integral ENA flux (0.1-60 keV) with no mass and energy resolution but relatively high angular resolution. The neutral particle detector (NPD) provides measurements of the ENA flux, resolving velocity (0.1-10 keV) and mass (H and O) with a coarse angular resolution. The electron spectrometer (ELS) is a standard top-hat electrostatic analyser in a very compact design. These three sensors are located on a scanning platform providing a 4 π coverage. The instrument also contains an ion mass composition sensor, IMA (ion mass analyser). Mechanically, IMA is a separate unit electrically connected with the ASPERA-4 main unit. IMA provides ion measurements in the energy range 0.01-36 keV/q for the main ion components H+, He++, He+, and the ion group with M / q 20 - 80 amu / q.

AB - The general scientific objective of the ASPERA-4 (Analyser of Space Plasmas and Energetic Atoms) experiment is to study the solar wind-atmosphere interaction and characterise the plasma and neutral gas environment in the near-Venus space through energetic neutral atom (ENA) imaging and local charged particle measurements. The studies to be performed address the fundamental question: How strongly do the interplanetary plasma and electromagnetic fields affect the Venusian atmosphere? The ASPERA-4 instrument comprises four sensors; two ENA sensors, electron and ion spectrometers. The neutral particle imager (NPI) provides measurements of the integral ENA flux (0.1-60 keV) with no mass and energy resolution but relatively high angular resolution. The neutral particle detector (NPD) provides measurements of the ENA flux, resolving velocity (0.1-10 keV) and mass (H and O) with a coarse angular resolution. The electron spectrometer (ELS) is a standard top-hat electrostatic analyser in a very compact design. These three sensors are located on a scanning platform providing a 4 π coverage. The instrument also contains an ion mass composition sensor, IMA (ion mass analyser). Mechanically, IMA is a separate unit electrically connected with the ASPERA-4 main unit. IMA provides ion measurements in the energy range 0.01-36 keV/q for the main ion components H+, He++, He+, and the ion group with M / q 20 - 80 amu / q.

KW - Energetic neutral atom imagers

KW - Ion and electron analysers

KW - Space instrumentation

KW - Venus

UR - http://www.scopus.com/inward/record.url?scp=34250724368&partnerID=8YFLogxK

U2 - 10.1016/j.pss.2007.01.014

DO - 10.1016/j.pss.2007.01.014

M3 - Article

AN - SCOPUS:34250724368

SN - 0032-0633

VL - 55

SP - 1772

EP - 1792

JO - Planetary and Space Science

JF - Planetary and Space Science

IS - 12

ER -

The Analyser of Space Plasmas and Energetic Atoms (ASPERA-4) for the Venus Express mission

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