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First results from the Solar Orbiter Heavy Ion SensorAims. 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.
Document ID
20230012783
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
S. Livi
(Southwest Research Institute San Antonio, United States)
S. T. Lepri
(University of Michigan–Ann Arbor Ann Arbor, United States)
J. M. Raines
(University of Michigan–Ann Arbor Ann Arbor, United States)
R. M. Dewey
(University of Michigan–Ann Arbor Ann Arbor, United States)
Antoinette B. Galvin
(University of New Hampshire Durham, United States)
P. Louarn
(Research Institute in Astrophysics and Planetology Toulouse, France)
Melissa R. Collier
(Bay Systems Consulting Greenbelt, United States)
Frederic Allegrini
(Southwest Research Institute San Antonio, United States)
B. L. Alterman
(Southwest Research Institute San Antonio, United States)
C. M. Bert
(University of Michigan–Ann Arbor Ann Arbor, United States)
R. Bruno
(National Institute for Astrophysics Rome, Italy)
Dennis J. Chornay
(University of Maryland, College Park College Park, United States)
R. D’Amicis ORCID
(National Institute for Astrophysics Rome, Italy)
T. J. Eddy
(University of Michigan–Ann Arbor Ann Arbor, United States)
L. Ellis
(University of New Hampshire Durham, United States)
E. Fauchon-Jones
(Imperial College London London, United Kingdom)
A. Fedorov
(Research Institute in Astrophysics and Planetology Toulouse, France)
I. Gershkovich
(University of Michigan–Ann Arbor Ann Arbor, United States)
J. Holmes
(University of Michigan–Ann Arbor Ann Arbor, United States)
T. S. Horbury
(Imperial College London London, United Kingdom)
Lynn M. Kistler
(University of New Hampshire Durham, United States)
Harald A. Kucharek
(University of New Hampshire Durham, United States)
N. Lugaz
(University of New Hampshire Durham, United States)
Teresa Nieves-Chinchilla
(Goddard Space Flight Center Greenbelt, United States)
H. O’Brien
(Imperial College London London, United Kingdom)
K. Ogasawara
(Southwest Research Institute San Antonio, United States)
C. J. Owen
(University College London London, United Kingdom)
M. Phillips
(Southwest Research Institute San Antonio, United States)
K. Ploof
(University of Michigan–Ann Arbor Ann Arbor, United States)
Y. J. Rivera
(Center for Astrophysics Harvard & Smithsonian Cambridge, Massachusetts, United States)
S. A. Spitzer
(University of Michigan–Ann Arbor Ann Arbor, United States)
Timothy J. Stubbs
(Goddard Space Flight Center Greenbelt, United States)
P. Wurz
(University of Bern Bern, Switzerland)
Date Acquired
August 30, 2023
Publication Date
August 2, 2023
Publication Information
Publication: Astronomy & Astrophysics
Publisher: EDP Sciences
Volume: 676
Issue Publication Date: August 1, 2023
ISSN: 0004-6361
e-ISSN: 1432-0746
Subject Category
Astronomy
Astrophysics
Funding Number(s)
WBS: 996805.04.01.01
CONTRACT_GRANT: NNN06AA01C
CONTRACT_GRANT: 80GSFC21M0002
CONTRACT_GRANT: NNG17FC93C
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
solar wind
heliosphere
general
particle emission
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