Solar physics in the 2020s: DKIST, parker solar probe, and solar orbiter as a multi-messenger constellation

Date Issued
2020
Author(s)
Martinez Pillet, V.
•
Tritschler, A.
•
Harra, L.
•
•
Vourlidas, A.
•
Raouafi, N.
•
Alterman, B. L.
•
Bellot Rubio, L.
•
•
Cranmer, S. R.
•
Gibson, S.
•
Habbal, S.
•
Ko, Y. K.
•
Lepri, S. T.
•
Linker, J.
•
Malaspina, D. M.
•
Matthews, S.
•
Parenti, S.
•
Petrie, G.
•
•
Ugarte-Urra, I.
•
Warren, H.
•
Winslow, R.
DOI
Abstract
The National Science Foundation (NSF) Daniel K. Inouye Solar Telescope (DKIST) is about to start operations at the summit of Haleakala (Hawaii). DKIST will join the early 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 detail remote observations of multiple layers of the Sun, the three observatories form an unprecedented multi-messenger constellation to study the magnetic connectivity inside the solar system. This white paper outlines the synergistic science that this multi-messenger suite enables.
Uri
Url
Ads BibCode
2020arXiv200408632M
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

2004.08632.pdf

Description
White Paper on arXiv
Size

706.03 KB

Format

Adobe PDF

Checksum (MD5)

56139e90faea01a33ef4463717371b22