First results from the Solar Orbiter Heavy Ion Sensor

被引：16

作者：

Livi, S. ^{[1
,2
]}

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

Raines, J. M. ^{[2
]}

Dewey, R. M. ^{[2
]}

Galvin, A. B. ^{[8
]}

Louarn, P. ^{[7
]}

Collier, M. R. ^{[4
]}

Allegrini, F. ^{[1
]}

Alterman, B. L. ^{[1
]}

Bert, C. M. ^{[2
]}

Bruno, R. ^{[11
]}

Chornay, D. J. ^{[4
]}

D'Amicis, R. ^{[11
]}

Eddy, T. J. ^{[2
]}

Ellis, L. ^{[8
]}

Fauchon-Jones, E. ^{[10
]}

Fedorov, A. ^{[7
]}

Gershkovich, I. ^{[2
]}

Holmes, J. ^{[2
]}

Horbury, T. S. ^{[10
]}

Kistler, L. M. ^{[8
]}

Kucharek, H. ^{[8
]}

Lugaz, N. ^{[8
]}

Nieves-Chinchilla, T. ^{[12
]}

O'Brien, H. ^{[10
]}

Ogasawara, K. ^{[1
]}

Owen, C. J. ^{[9
]}

Phillips, M. ^{[1
]}

Ploof, K. ^{[2
]}

Rivera, Y. J. ^{[3
]}

Spitzer, S. A. ^{[2
]}

Stubbs, T. J. ^{[5
]}

Wurz, P. ^{[6
]}

机构：

[1] Southwest Res Inst, Space Sci & Engn, 6220 Culebra Rd, San Antonio, TX 78238 USA

[2] Univ Michigan, Dept Climate & Space Sci & Engn, Climate & Space Res Bldg,2455 Hayward St, Ann Arbor, MI 48109 USA

[3] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[4] NASA Goddard Space Flight Ctr, Heliophys Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[5] NASA Goddard Space Flight Ctr, Solar Syst Explorat Div, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[6] Univ Bern, Phys Inst, Sidlerstr 5, CH-3012 Bern, Switzerland

[7] Inst Rech Astrophys & Planetol, 9 Ave Colonel ROCHE,BP 4346, F-31028 Toulouse 4, France

[8] Univ New Hampshire, Space Sci Ctr, 8 Coll Rd, Durham, NH 03824 USA

[9] Univ Coll London, Dept Space & Climate Phys, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England

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

[11] INAF IFSI, Via Fosso del Cavaliere 100, I-00133 Rome, Italy

[12] NASA Goddard Space Flight Ctr, Heliospher Phys Lab, Heliophys Sci Div, 8800 Greenbelt Rd, Greenbelt, MD 20770 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2023年 / 676卷

关键词：

solar wind; Sun; heliosphere; general; particle emission; CORONAL MASS EJECTIONS; PICKUP IONS; VELOCITY DISTRIBUTION; ELEMENTAL ABUNDANCES; JANUARY; 6; AU; WIND; ORIGIN; IONIZATION; INTERSTELLAR;

D O I：

10.1051/0004-6361/202346304

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Aims. Solar Orbiter launched in February 2020 with the goal of revealing the connections between the Sun's interior, atmosphere, and the heliosphere. The Solar Orbiter Heavy Ion Sensor (HIS) is a time-of-flight ion mass spectrometer dedicated to measuring heavy ions in the solar wind.Methods. We present an overview of the first measurements of heavy ion composition from HIS, reviewing the methods used to transform the spectra obtained on board into scientific data products and examining two solar wind case studies as well as the statistical properties of the heavy ion composition observed by HIS. We also carried out a comparison with prior measurements of heavy ions at L1.Results. The HIS data set provides the first mass- and charge-resolved heavy ion measurements in the inner heliosphere.Conclusions. These high temporal resolution data have the potential to transform our understanding of the connections between the solar wind and its origin at the Sun, as well as the interaction between the solar wind and the environment around planets, comets, and in the interstellar medium.

引用

页数：14

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