Solar orbiter neutral solar-wind detector

M. Hilchenbach; S. Orsini; K. C. Hseih; E. Antonucci; S. Barabash; K. Bamert; R. Bruno; M. R. Collier; A. Czechowski; R. D'Amicis; E. De Angelis; I. Dandouras; A. M. Di Lellis; R. Esser; J. Giacalone; M. Gruntman; S. R. Habbal; J. R. Jokipii; E. Kallio; J. Kota; H. Kucharek; R. Leonl; S. Livi; I. Mann; E. Marsch; S. Massetti; A. Milillo; E. Möbius; A. Mura; R. B. Sheldon; W. Schmidt; S. Selci; K. Szego; J. Woch; P. Wurz; V. Zanza; T. H. Zurbuchen

Solar orbiter neutral solar-wind detector

M. Hilchenbach^*, S. Orsini, K. C. Hseih, E. Antonucci, S. Barabash, K. Bamert, R. Bruno, M. R. Collier, A. Czechowski, R. D'Amicis, E. De Angelis, I. Dandouras, A. M. Di Lellis, R. Esser, J. Giacalone, M. Gruntman, S. R. Habbal, J. R. Jokipii, E. Kallio, J. KotaH. Kucharek, R. Leonl, S. Livi, I. Mann, E. Marsch, S. Massetti, A. Milillo, E. Möbius, A. Mura, R. B. Sheldon, W. Schmidt, S. Selci, K. Szego, J. Woch, P. Wurz, V. Zanza, T. H. Zurbuchen

^*Corresponding author for this work

Not published at Aalto University

Research output: Chapter in Book/Report/Conference proceeding › Conference article in proceedings › Scientific › peer-review

Abstract

Neutral hydrogen atoms, which give rise to the prominent solar Ly-α corona, are closely coupled to the emerging solar-wind plasma. The density ratio of neutral hydrogen to protons is minute, ∼10^-6; therefore, the neutral atoms are tracers in the solar wind. In-situ observations of the neutral atoms, their flight paths (imaging), density, and velocity distributions are a new tool to the understanding of the Ly-α corona, i.e. setting limits on the plasma velocity distribution along the solar magnetic field lines. The other goal of the neutral solar-wind instrumentation is the in-situ observation of the interactions between solar wind plasma and dust grains near the Sun. We will discuss the science objectives and the potential "zero charge" solar-wind instrument envelope onboard Solar Orbiter.

Original language	English
Title of host publication	Proceedings of the Second Solar Orbiter Workshop
Edition	SP-641
Publication status	Published - Oct 2006
MoE publication type	A4 Conference publication
Event	Solar Orbiter Workshop - Athens, Greece Duration: 16 Oct 2006 → 20 Oct 2006 Conference number: 2

Publication series

Name	European Space Agency, (Special Publication) ESA SP
Number	SP-641
ISSN (Print)	0379-6566

Workshop

Workshop	Solar Orbiter Workshop
Country/Territory	Greece
City	Athens
Period	16/10/2006 → 20/10/2006

Cite this

Hilchenbach, M., Orsini, S., Hseih, K. C., Antonucci, E., Barabash, S., Bamert, K., Bruno, R., Collier, M. R., Czechowski, A., D'Amicis, R., De Angelis, E., Dandouras, I., Di Lellis, A. M., Esser, R., Giacalone, J., Gruntman, M., Habbal, S. R., Jokipii, J. R., Kallio, E., ... Zurbuchen, T. H. (2006). Solar orbiter neutral solar-wind detector. In Proceedings of the Second Solar Orbiter Workshop (SP-641 ed.). (European Space Agency, (Special Publication) ESA SP; No. SP-641).

@inproceedings{62ade9a7358c49c2a05c3508da2831f8,

title = "Solar orbiter neutral solar-wind detector",

abstract = "Neutral hydrogen atoms, which give rise to the prominent solar Ly-α corona, are closely coupled to the emerging solar-wind plasma. The density ratio of neutral hydrogen to protons is minute, ∼10-6; therefore, the neutral atoms are tracers in the solar wind. In-situ observations of the neutral atoms, their flight paths (imaging), density, and velocity distributions are a new tool to the understanding of the Ly-α corona, i.e. setting limits on the plasma velocity distribution along the solar magnetic field lines. The other goal of the neutral solar-wind instrumentation is the in-situ observation of the interactions between solar wind plasma and dust grains near the Sun. We will discuss the science objectives and the potential {"}zero charge{"} solar-wind instrument envelope onboard Solar Orbiter.",

author = "M. Hilchenbach and S. Orsini and Hseih, {K. C.} and E. Antonucci and S. Barabash and K. Bamert and R. Bruno and Collier, {M. R.} and A. Czechowski and R. D'Amicis and {De Angelis}, E. and I. Dandouras and {Di Lellis}, {A. M.} and R. Esser and J. Giacalone and M. Gruntman and Habbal, {S. R.} and Jokipii, {J. R.} and E. Kallio and J. Kota and H. Kucharek and R. Leonl and S. Livi and I. Mann and E. Marsch and S. Massetti and A. Milillo and E. M{\"o}bius and A. Mura and Sheldon, {R. B.} and W. Schmidt and S. Selci and K. Szego and J. Woch and P. Wurz and V. Zanza and Zurbuchen, {T. H.}",

year = "2006",

month = oct,

language = "English",

isbn = "9290922052",

series = "European Space Agency, (Special Publication) ESA SP",

number = "SP-641",

booktitle = "Proceedings of the Second Solar Orbiter Workshop",

edition = "SP-641",

note = "Solar Orbiter Workshop ; Conference date: 16-10-2006 Through 20-10-2006",

}

Hilchenbach, M, Orsini, S, Hseih, KC, Antonucci, E, Barabash, S, Bamert, K, Bruno, R, Collier, MR, Czechowski, A, D'Amicis, R, De Angelis, E, Dandouras, I, Di Lellis, AM, Esser, R, Giacalone, J, Gruntman, M, Habbal, SR, Jokipii, JR, Kallio, E, Kota, J, Kucharek, H, Leonl, R, Livi, S, Mann, I, Marsch, E, Massetti, S, Milillo, A, Möbius, E, Mura, A, Sheldon, RB, Schmidt, W, Selci, S, Szego, K, Woch, J, Wurz, P, Zanza, V & Zurbuchen, TH 2006, Solar orbiter neutral solar-wind detector. in Proceedings of the Second Solar Orbiter Workshop. SP-641 edn, European Space Agency, (Special Publication) ESA SP, no. SP-641, Solar Orbiter Workshop, Athens, Greece, 16/10/2006.

TY - GEN

T1 - Solar orbiter neutral solar-wind detector

AU - Hilchenbach, M.

AU - Orsini, S.

AU - Hseih, K. C.

AU - Antonucci, E.

AU - Barabash, S.

AU - Bamert, K.

AU - Bruno, R.

AU - Collier, M. R.

AU - Czechowski, A.

AU - D'Amicis, R.

AU - De Angelis, E.

AU - Dandouras, I.

AU - Di Lellis, A. M.

AU - Esser, R.

AU - Giacalone, J.

AU - Gruntman, M.

AU - Habbal, S. R.

AU - Jokipii, J. R.

AU - Kallio, E.

AU - Kota, J.

AU - Kucharek, H.

AU - Leonl, R.

AU - Livi, S.

AU - Mann, I.

AU - Marsch, E.

AU - Massetti, S.

AU - Milillo, A.

AU - Möbius, E.

AU - Mura, A.

AU - Sheldon, R. B.

AU - Schmidt, W.

AU - Selci, S.

AU - Szego, K.

AU - Woch, J.

AU - Wurz, P.

AU - Zanza, V.

AU - Zurbuchen, T. H.

N1 - Conference code: 2

PY - 2006/10

Y1 - 2006/10

N2 - Neutral hydrogen atoms, which give rise to the prominent solar Ly-α corona, are closely coupled to the emerging solar-wind plasma. The density ratio of neutral hydrogen to protons is minute, ∼10-6; therefore, the neutral atoms are tracers in the solar wind. In-situ observations of the neutral atoms, their flight paths (imaging), density, and velocity distributions are a new tool to the understanding of the Ly-α corona, i.e. setting limits on the plasma velocity distribution along the solar magnetic field lines. The other goal of the neutral solar-wind instrumentation is the in-situ observation of the interactions between solar wind plasma and dust grains near the Sun. We will discuss the science objectives and the potential "zero charge" solar-wind instrument envelope onboard Solar Orbiter.

AB - Neutral hydrogen atoms, which give rise to the prominent solar Ly-α corona, are closely coupled to the emerging solar-wind plasma. The density ratio of neutral hydrogen to protons is minute, ∼10-6; therefore, the neutral atoms are tracers in the solar wind. In-situ observations of the neutral atoms, their flight paths (imaging), density, and velocity distributions are a new tool to the understanding of the Ly-α corona, i.e. setting limits on the plasma velocity distribution along the solar magnetic field lines. The other goal of the neutral solar-wind instrumentation is the in-situ observation of the interactions between solar wind plasma and dust grains near the Sun. We will discuss the science objectives and the potential "zero charge" solar-wind instrument envelope onboard Solar Orbiter.

UR - http://www.scopus.com/inward/record.url?scp=34249688662&partnerID=8YFLogxK

M3 - Conference article in proceedings

AN - SCOPUS:34249688662

SN - 9290922052

SN - 9789290922056

T3 - European Space Agency, (Special Publication) ESA SP

BT - Proceedings of the Second Solar Orbiter Workshop

T2 - Solar Orbiter Workshop

Y2 - 16 October 2006 through 20 October 2006

ER -

Solar orbiter neutral solar-wind detector

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