http://www.cnr.it/ontology/cnr/individuo/prodotto/ID241097

Solar Orbiter Neutral Solar Wind Detector (Contributo in atti di convegno)

Type

Label

Solar Orbiter Neutral Solar Wind Detector (Contributo in atti di convegno) (literal)

Anno

Alternative label

M. Hilchenbach (1); S. Orsini (2); K.C. Hsieh (3); E. Antonucci (4); S. Barabash (5); K. Bamert (6); R. Bruno (2); M.R. Collier (7); A. Czechowski (8); R. D'Amicis (2); E. De Angelis (2); I. Dandouras (9); A.M. Di Lellis (10); R. Esser (11); J. Giacalone (3); M. Gruntman (12); S.R. Habbal (13); J.R. Jokipii (3); E. Kallio (14); J. Kota (3); H. Kucharek (15); R. Leoni (16); S. Livi (17); I. Mann (18); E. Marsch (1); S. Massetti (2); A. Milillo (2); E. Möbius (15); A. Mura (2); R.B. Sheldon (19); W. Schmidt (14); S. Selci (20); K. Szego (21); J. Woch (1); P. Wurz (6); V. Zanza (22); T.H. Zurbuchen (23) (2007)
Solar Orbiter Neutral Solar Wind Detector
in The Second Solar Orbiter Workshop, Athens, Greece, 16-20 October 200
(literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori

M. Hilchenbach (1); S. Orsini (2); K.C. Hsieh (3); E. Antonucci (4); S. Barabash (5); K. Bamert (6); R. Bruno (2); M.R. Collier (7); A. Czechowski (8); R. D'Amicis (2); E. De Angelis (2); I. Dandouras (9); A.M. Di Lellis (10); R. Esser (11); J. Giacalone (3); M. Gruntman (12); S.R. Habbal (13); J.R. Jokipii (3); E. Kallio (14); J. Kota (3); H. Kucharek (15); R. Leoni (16); S. Livi (17); I. Mann (18); E. Marsch (1); S. Massetti (2); A. Milillo (2); E. Möbius (15); A. Mura (2); R.B. Sheldon (19); W. Schmidt (14); S. Selci (20); K. Szego (21); J. Woch (1); P. Wurz (6); V. Zanza (22); T.H. Zurbuchen (23) (literal)

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(1) Max-Planck Institute, Germany (2) IFSI/CNR Via Fosso del Cavaliere, Roma [poi INAF] (3) University of Arizona, Tucson, USA (4) Osservatorio Astronimico di Torino (5) RF- Swedish Institute Of Space Physics, Sweden (6) Physikalisches Institut, Space Research & Planetary Sciences, Bern, Switzerland (7) Interplanetary Physics NASA/Goddard Space ... Maryland, USA (8) Space Research Center, Warsaw, Poland (9) Centre d'Etude Spatiale des Rayonnements CESR, Toulouse, France (10) AMDL s.r.l., Roma (11) Dept. of Physics, Univ. of Tromso, Norway (12) Viterbi School of Engineering, Downey (13) Univ. of Southern California, Los Angeles, USA (14) Finnish Meteorological Institute, Helsinki, Finland (15) Dep. of Physics, Univ. of New Hampshire, Durham, USA (16) IFN/CNR, Roma (17) JHU/APL, Laurel, USA (18) Dept. of Earth and Planetary Science, Kobe Univ., Japan (19) NASA/MSFC/NSSTC/VP62, Huntsville, USA (20) ISC/CNR, via Fosso del Cavaliere, Roma (21) KFKI, Hungarian Academy of Sciences, Budapest, Hungary (22) ENEA, Frascati (23) Dept. of Atmospheric, Oceanic and Space Science, Univ. of Michigan, USA (literal)

Titolo

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Abstract

Neutral hydrogen atoms, which give rise to the prominent so lar Ly-alpha corona, are closely coup led 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 (imag ing), density, and velocity distribu tions are a new tool to the understanding of the Ly-alpha 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. (literal)

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