Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum

被引：84

作者：

Raouafi, N. E. ^{[1
]}

Matteini, L. ^{[2
]}

Squire, J. ^{[3
]}

Badman, S. T. ^{[4
,5
]}

Velli, M. ^{[6
]}

Klein, K. G. ^{[7
]}

Chen, C. H. K. ^{[8
]}

Matthaeus, W. H. ^{[9
]}

Szabo, A. ^{[10
]}

Linton, M. ^{[11
]}

Allen, R. C. ^{[1
]}

Szalay, J. R. ^{[12
]}

Bruno, R. ^{[13
]}

Decker, R. B. ^{[1
]}

Akhavan-Tafti, M. ^{[14
]}

Agapitov, O. V. ^{[5
]}

Bale, S. D. ^{[5
,15
]}

Bandyopadhyay, R. ^{[12
]}

Battams, K. ^{[11
]}

Bercic, L. ^{[16
]}

Bourouaine, S. ^{[1
]}

Bowen, T. A. ^{[5
]}

Cattell, C. ^{[17
]}

Chandran, B. D. G. ^{[18
,19
]}

Chhiber, R. ^{[9
,10
]}

Cohen, C. M. S. ^{[20
]}

D'Amicis, R. ^{[13
]}

Giacalone, J. ^{[7
]}

Hess, P. ^{[11
]}

Howard, R. A. ^{[1
]}

Horbury, T. S. ^{[2
]}

Jagarlamudi, V. K. ^{[1
]}

Joyce, C. J. ^{[21
]}

Kasper, J. C. ^{[14
,22
]}

Kinnison, J. ^{[1
]}

Laker, R. ^{[2
]}

Liewer, P. ^{[23
]}

Malaspina, D. M. ^{[24
,25
]}

Mann, I. ^{[26
]}

McComas, D. J. ^{[12
]}

Niembro-Hernandez, T. ^{[4
]}

Nieves-Chinchilla, T. ^{[10
]}

Panasenco, O. ^{[27
]}

Pokorny, P. ^{[28
,29
,30
]}

Pusack, A. ^{[25
]}

Pulupa, M. ^{[5
]}

Perez, J. C. ^{[31
]}

Riley, P. ^{[32
]}

Rouillard, A. P. ^{[33
]}

Shi, C. ^{[6
]}

机构：

[1] Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA

[2] Imperial Coll London, Dept Phys, South Kensington Campus, London SW7 2AZ, England

[3] Univ Otago, Phys Dept, Dunedin 9010, New Zealand

[4] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA

[5] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[6] UCLA, Earth Planetary & Space Sci, Los Angeles, CA 90095 USA

[7] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA

[8] Queen Mary Univ London, Dept Phys & Astron, London E1 4NS, England

[9] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA

[10] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[11] Naval Res Lab, Space Sci Div, Washington, DC 20375 USA

[12] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08540 USA

[13] Inst Space Astrophys & Planetol IAPS, Natl Inst Astrophys INAF, I-00133 Rome, Italy

[14] Univ Michigan, Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA

[15] Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA

[16] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

[17] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN USA

[18] Univ New Hampshire, Dept Phys & Astron, Durham, NH USA

[19] Univ New Hampshire, Space Sci Ctr, Durham, NH 03824 USA

[20] CALTECH, Pasadena, CA 91125 USA

[21] Univ New Hampshire, Durham, NH 03824 USA

[22] BWX Technol Inc, Washington, DC 20002 USA

[23] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[24] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA

[25] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80303 USA

[26] Dept Phys & Technol, Postboks 6050, N-9037 Tromso, Norway

[27] Adv Heliophys, Pasadena, CA 91106 USA

[28] NASA, Astrophys Sci Div, Goddard Spaceflight Ctr, Greenbelt, MD 20771 USA

[29] Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA

[30] NASA, Ctr Res & Explorat Space Sci & Technol, GSFC, Greenbelt, MD 20771 USA

[31] Florida Inst Technol, Dept Aerosp Phys & Space Sci, Melbourne, FL 32901 USA

[32] Predict Sci Inc, San Diego, CA USA

[33] Univ Toulouse, IRAP, CNRS, CNES,UPS, Toulouse, France

[34] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA

来源：

SPACE SCIENCE REVIEWS | 2023年 / 219卷 / 01期

关键词：

Sun; Corona; Solar wind; Plasma; Magnetic fields; Coronal mass ejections; Parker solar probe; CORONAL MASS EJECTIONS; ANOMALOUS COSMIC-RAYS; MAGNETIC-FLUX ROPES; CIRCUMSOLAR DUST RING; COROTATING INTERACTION REGIONS; ELECTRON-CYCLOTRON FREQUENCY; ENERGETIC PARTICLE EVENTS; CO-ORBITAL ASTEROIDS; ION-ACOUSTIC-WAVES; CIRCLE-DOT-IS;

D O I：

10.1007/s11214-023-00952-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to determine the structure and dynamics of the Sun's coronal magnetic field, understand how the solar corona and wind are heated and accelerated, and determine what processes accelerate energetic particles. Parker Solar Probe returned a treasure trove of science data that far exceeded quality, significance, and quantity expectations, leading to a significant number of discoveries reported in nearly 700 peer-reviewed publications. The first four years of the 7-year primary mission duration have been mostly during solar minimum conditions with few major solar events. Starting with orbit 8 (i.e., 28 Apr. 2021), Parker flew through the magnetically dominated corona, i.e., sub-Alfvenic solar wind, which is one of the mission's primary objectives. In this paper, we present an overview of the scientific advances made mainly during the first four years of the Parker Solar Probe mission, which go well beyond the three science objectives that are: (1) Trace the flow of energy that heats and accelerates the solar corona and solar wind; (2) Determine the structure and dynamics of the plasma and magnetic fields at the sources of the solar wind; and (3) Explore mechanisms that accelerate and transport energetic particles.

引用

页数：140

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