SH032
Utilizing Next Generation Helio Missions to Address Long Standing Solar Wind Mysteries

Session ID#: 80625

Session Description:
Many in situ quantities are not conserved along solar wind propagation and the processes contributing to this evolution are poorly understood. While the connection between solar phenomena and in situ measurements is opaque, these observations carry clues about the plasma’s solar origin. The recent release of Parker Solar Probe data and upcoming Solar Orbiter, DKIST, and IMAP measurements will enable the heliospheric and solar communities to quantifiably connect in situ and remote observations. This session will discuss leveraging data, theory, and modeling to answer: 1) How can in situ measurements together with remote observations characterize solar wind acceleration and heating? 2) How can conserved (e.g. charge states, abundances) and non-conserved quantities (e.g. VDFs, temperature anisotropies) be jointly leveraged to probe transport effects? 3) How can theory and modeling disentangle propagation effects from signatures of solar sources? 4) What new multi-messenger studies would significantly advance these efforts?
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7859 Transport processes [SPACE PLASMA PHYSICS]

Primary Convener:  Yeimy Rivera, University of Michigan Ann Arbor, Ann Arbor, MI, United States
Conveners:  Benjamin L Alterman, University of Michigan, Ann Arbor, MI, United States, Aleida Katherine Higginson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Steven R Cranmer, University of Colorado at Boulder, APS, Boulder, CO, United States
Primary Liaison:  Yeimy Rivera, University of Michigan Ann Arbor, Ann Arbor, MI, United States
 
DKIST, PARKER SOLAR PROBE (PSP), AND SOLAR ORBITER AS A MULTI-MESSENGER CONSTELLATION (Invited) (486173)
Valentin Martinez Pillet, National Solar Observatory, Tucson, AZ, United States and DKIST CSP APL Workshop Participants
 
Modeling Solar Wind Connectivity from Origin to Detection (Invited) (491655)
Samantha Wallace1, Charles Nickolos Arge2, Shaela I Jones2, Carl J Henney3 and Adam Szabo2, (1)University of New Mexico Main Campus, Albuquerque, NM, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, NM, United States
 
The multi-messenger era enabled by DKIST, PSP, and Solar Orbiter (507915)
Valentin Martinez Pillet, National Solar Observatory, Tucson, AZ, United States
 
Transient coronal heating as a source of density fluctuations imaged by STEREO and future space missions (536559)
Léa Sophie Griton1, Rui Pinto2, Alexis P Rouillard2 and Michael Lavarra3, (1)IRAP, CNRS, Université Paul Sabatier, Toulouse, France, (2)IRAP/CNRS, Toulouse, France, (3)IRAP, Toulouse, France
 
Investigating the role of solar wind-dust interaction in the production of He+ (546940)
Yeimy Rivera1, Enrico Landi2, Susan T Lepri2 and Sarah A. Spitzer1, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, MI, United States
 
LOCKYER: Large Optimized Coronagraphs for KeY Emission line Research (588308)
John Martin Laming, US Naval Research Laboratory, Washington, DC, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and LOCKYER Team
See more of: SPA-Solar and Heliospheric Physics
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