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Solar Physics in the 2020s: DKIST, Parker Solar Probe, and Solar Orbiter as a Multi-Messenger Constellation

Published online by Cambridge University Press:  28 September 2023

V. Martinez Pillet Open the ORCID record for V. Martinez Pillet [Opens in a new window] ,
G. Cauzzi Open the ORCID record for G. Cauzzi [Opens in a new window] ,
A. Tritschler ,
L. Harra ,
V. Andretta ,
A. Vourlidas ,
N. Raouafi ,
B. L. Alterman ,
L. Bellot Rubio  and
S. R. Cranmer
...Show all authors
V. Martinez Pillet
Affiliation:
National Solar Observatory, Boulder, CO, USA
G. Cauzzi
Affiliation:
National Solar Observatory, Boulder, CO, USA
A. Tritschler
Affiliation:
National Solar Observatory, Boulder, CO, USA
L. Harra
Affiliation:
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center & ETH-Zürich, Switzerland
V. Andretta
Affiliation:
INAF/OACN, Italy
A. Vourlidas
Affiliation:
Johns Hopkins University Applied Physics Lab, MD, USA
N. Raouafi
Affiliation:
Johns Hopkins University Applied Physics Lab, MD, USA
B. L. Alterman
Affiliation:
Space Science and Engineering, Southwest Research Institute, San Antonio, TX, USA
L. Bellot Rubio
Affiliation:
Instituto de Astrof sica de Andalucia, Granada, Spain
S. R. Cranmer
Affiliation:
Department of Astrophysical and Planetary Sciences, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA
S. Gibson
Affiliation:
High Altitude Observatory, NCAR, Boulder, CO, USA
A. De Groof
Affiliation:
European Space Agency, European Space Astronomy Centre, Madrid, Spain
Y.-K. Ko
Affiliation:
Space Science Division, US Naval Research Laboratory, Washington, D.C., USA
S. T. Lepri
Affiliation:
Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA
J. Linker
Affiliation:
Predictive Science Inc., San Diego, CA, USA
D. M. Malaspina
Affiliation:
Department of Astrophysical and Planetary Sciences, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA
S. Matthews
Affiliation:
UCL Mullard Space Science Laboratory, UK
D. Müller
Affiliation:
European Space Agency, European Space Research and Technology Centre, Noordwijk, The Netherlands
S. Parenti
Affiliation:
Université Paris-Saclay, CNRS, Institut d’astrophysique spatiale, 91405, Orsay, France
G. Petrie
Affiliation:
National Solar Observatory, Boulder, CO, USA
D. Spadaro
Affiliation:
INAF/OACT, Italy
I. Ugarte-Urra
Affiliation:
Space Science Division, US Naval Research Laboratory, Washington, D.C., USA
H. Warren
Affiliation:
Space Science Division, US Naval Research Laboratory, Washington, D.C., USA
I. Zouganelis
Affiliation:
European Space Agency, European Space Astronomy Centre, Madrid, Spain
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Abstract

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The National Science Foundation (NSF) Daniel K. Inouye Solar Telescope (DKIST) has started operations at the summit of Haleakalā (Hawai’i). DKIST joins the nominal science phases of the NASA and ESA Parker Solar Probe and Solar Orbiter encounter missions. By combining in-situ measurements of the near-Sun plasma environment and detailed remote observations of multiple layers of the Sun, the three observatories form an unprecedented multi-messenger constellation to study the magnetic connectivity in the solar system. This work outlines the synergistic science that this multi-messenger suite enables.

Keywords

Sun: generalSun: atmosphereSun: magnetic fields(Sun:) solar wind
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S372: The Era of Multi-Messenger Solar Physics , August 2022 , pp. 3 - 16
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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