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

V. Martinez Pillet, G. Cauzzi, A. Tritschler, L. Harra, V. Andretta, A. Vourlidas, N. Raouafi, B. L. Alterman, L. Bellot Rubio, S. R. Cranmer, S. Gibson, A. De Groof, Y. K. Ko, S. T. Lepri, J. Linker, D. M. Malaspina, S. Matthews, D. Müller, S. Parenti, G. PetrieD. Spadaro, I. Ugarte-Urra, H. Warren, I. Zouganelis

Research output: Chapter in Book/Report/Conference proceedingChapterpeer-review

2 Scopus citations

Abstract

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.

Original languageEnglish
Title of host publicationProceedings of the International Astronomical Union
EditorsG. Cauzzi, A. Tritschler
PublisherCambridge University Press
Pages3-16
Number of pages14
DOIs
StatePublished - Aug 28 2022

Publication series

NameProceedings of the International Astronomical Union
Volume18
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • (Sun:) solar wind
  • Sun: atmosphere
  • Sun: general
  • Sun: magnetic fields

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