Beam tracking strategies for fast acquisition of solar wind velocity distribution functions with high energy and angular resolutions
Autor: | Maria Federica Marcucci, Benoit Lavraud, Bram Beeckman, Lubomír Přech, Rossana De Marco, Eddy Neefs, Sophie Berkenbosch, Daniele Brienza, Johan De Keyser, Andrei Fedorov |
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Přispěvatelé: | Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS) |
Jazyk: | angličtina |
Rok vydání: | 2018 |
Předmět: |
Atmospheric Science
010504 meteorology & atmospheric sciences [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] Population 01 natural sciences Optics 0103 physical sciences Earth and Planetary Sciences (miscellaneous) Particle velocity education lcsh:Science 010303 astronomy & astrophysics 0105 earth and related environmental sciences Physics education.field_of_study Spectrometer Spacecraft business.industry lcsh:QC801-809 Geology Astronomy and Astrophysics lcsh:QC1-999 Solar wind lcsh:Geophysics. Cosmic physics Distribution function Space and Planetary Science Physics::Space Physics lcsh:Q business [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Energy (signal processing) Beam (structure) lcsh:Physics |
Zdroj: | Annales Geophysicae, Vol 36, Pp 1285-1302 (2018) Annales Geophysicae Annales Geophysicae, 2018, ⟨10.5194/angeo-36-1285-2018⟩ Annales Geophysicae, European Geosciences Union, 2018, ⟨10.5194/angeo-36-1285-2018⟩ |
ISSN: | 1432-0576 0992-7689 |
Popis: | Space plasma spectrometers have often relied on spacecraft spin to collect three-dimensional particle velocity distributions, which simplifies the instrument design and reduces its resource budgets but limits the velocity distribution acquisition rate. This limitation can in part be overcome by the use of electrostatic deflectors at the entrance of the analyser. By mounting such a spectrometer on a Sun-pointing spacecraft, solar wind ion distributions can be acquired at a much higher rate because the solar wind ion population, which is a cold beam that fills only part of the sky around its mean arrival direction, always remains in view. The present paper demonstrates how the operation of such an instrument can be optimized through the use of beam tracking strategies. The underlying idea is that it is much more efficient to cover only that part of the energy spectrum and those arrival directions where the solar wind beam is expected to be. The advantages of beam tracking are a faster velocity distribution acquisition for a given angular and energy resolution, or higher angular and energy resolution for a given acquisition rate. It is demonstrated by simulation that such beam tracking strategies can be very effective while limiting the risk of losing the beam. They can be implemented fairly easily with present-day on-board processing resources. |
Databáze: | OpenAIRE |
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