POLAR investigation of the Sun -- POLARIS
Creators
- Appourchaux, T.1
- Liewer, P.2
- Watt, M.
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Alexander, D.3
- Andretta, V.4
- Auchère, F.1
- D'Arrigo, P.
- Ayon, J.2
- Corbard, T.5
- Fineschi, S.4
- Finsterle, W.
- Floyd, L.
- Garbe, G.6
- Gizon, L.7
- Hassler, D.8
- Harra, L.
- Kosovichev, A.9
- Leibacher, J.1, 10
- Leipold, M.
- Murphy, N.2
- Maksimovic, M.11
- Martinez-Pillet, V.12
- Matthews, B. S. A.
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Mewaldt, R.13
- Moses, D.14
- Newmark, J.14
- Régnier, S.15
- Schmutz, W.
- Socker, D.14
- Spadaro, D.16
- Stuttard, D.
- Trosseille, C.1
- Ulrich, R.17
- Velli, M.2
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Vourlidas, A.14
- Wimmer-Schweingruber, C. R.18
- Zurbuchen, T.19
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1.
Institut d'Astrophysique Spatiale
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2.
Jet Propulsion Lab
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3.
Rice University
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4.
Astronomical Observatory of Capodimonte
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5.
Observatoire de la Côte d'Azur
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6.
National Space Science and Technology Center
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7.
Max Planck Institute for Solar System Research
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8.
Southwest Research Institute
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9.
Stanford University
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10.
Association of Universities For Research In Astronomy
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11.
Paris Observatory
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12.
Instituto de Astrofísica de Canarias
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13.
California Institute of Technology
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14.
United States Naval Research Laboratory
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15.
University of St Andrews
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16.
Osservatorio Astrofisico di Catania
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17.
University of California, Los Angeles
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18.
Kiel University
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19.
University of Michigan–Ann Arbor
Abstract
The POLAR Investigation of the Sun (POLARIS) mission uses a combination of a gravity assist and solar sail propulsion to place a spacecraft in a 0.48 AU circular orbit around the Sun with an inclination of 75° with respect to solar equator. This challenging orbit is made possible by the challenging development of solar sail propulsion. This first extended view of the high-latitude regions of the Sun will enable crucial observations not possible from the ecliptic viewpoint or from Solar Orbiter. While Solar Orbiter would give the first glimpse of the high latitude magnetic field and flows to probe the solar dynamo, it does not have sufficient viewing of the polar regions to achieve POLARIS's primary objective: determining the relation between the magnetism and dynamics of the Sun's polar regions and the solar cycle.
Additional Information
© The Authors 2009. This article is distributed under the terms of the Creative Commons Attribution Noncommercial License which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and source are credited. Received: 16 November 2007; Accepted: 3 June 2008; Published online: 12 July 2008.Attached Files
Published - Appourchaux2009p143Exp_Astron.pdf
Files
Appourchaux2009p143Exp_Astron.pdf
Additional details
Identifiers
- Eprint ID
- 14240
- Resolver ID
- CaltechAUTHORS:20090515-153035829
Dates
- Created
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2009-08-24Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Space Radiation Laboratory