410:
Next-Generation Solar Physics Missions III


Session ID#: 43063

Session Description:
In June 2016, a Next Generation Solar Physics Mission (NGSPM) study was chartered by NASA, JAXA, and ESA for a multilateral solar physics mission concept to bring closure to science objectives by exploring and exploiting new windows on, e.g., wavelength, continuity, spatial and temporal resolution, spectroscopy and polarimetry, vantage point and orbit, with due consideration given to readiness of technology and analysis methods. The resulting report (http://hinode.nao.ac.jp/SOLAR-C/SOLAR-C/Documents/NGSPM_report_170731.pdf ) presents recommendations for a future mission or missions that focus on the study of fundamental physical processes at high spatial and temporal resolution through all temperature regimes of the solar atmosphere. This special session will comprise invited talks that will overview the recommendations from the report, science enabled by the instruments recommended, and synergies between NGSPM recommendations and existing and planned observatories. Interested authors are also encouraged to submit abstracts on these and other topics encompassed in the report, including consideration of science enabled by multivantage observations.
Primary Convener:  David E. McKenzie, NASA Marshall Space Flight Center, Huntsville, AL, United States
Conveners:  Sarah E Gibson, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, Theodore D Tarbell, Lockheed Martin, Palo Alto, CA, United States and John C Raymond, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
Chairs:  David E. McKenzie, NASA Marshall Space Flight Center, Huntsville, AL, United States and Sarah E Gibson, National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States

Abstracts Submitted to this Session:

410.01
Recommendations from the NGSPM-SOT report and mission opportunities in Japan (Invited) (334449)
Toshifumi Shimizu, JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan
410.02
NASA Heliophysics Update (Invited) (334963)
Peg Luce, NASA Headquarters, Washington, DC, United States
410.03
A Next Generation Spectrometer: The EUV High-Throughput Spectroscopic Telescope (EUVST) (334396)
Harry P Warren, Naval Research Laboratory, Washington, DC, United States
410.04
An Innovative Approach to a High Resolution Coronal Imager (T-07): MUSE, the Multi-Slit Solar Explorer (335389)
Theodore D Tarbell and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
410.05
NGSPM Objectives Addressed by the FOXSI SMEX Mission (335405)
Albert Y Shih, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Steven Christe, NASA GSFC, Solar Physics Lab, Greenbelt, United States, Sam Krucker, ETH Zürich, Zurich, Switzerland, Lindsay Glesener, University of Minnesota Twin Cities, Minneapolis, United States, Pascal Saint-Hilaire, UC Berkeley, Space Science Lab, Berkeley, United States and Amir Caspi, Southwest Research Institute, Boulder, CO, United States
410.06
A Novel Soft X-ray Slitless Imaging Spectrograph for Unique Diagnostics of Hot Coronal Plasma (335930)
Amir Caspi1, Albert Y Shih2, Harry P Warren3, Thomas N Woods4, Dr. James Paul Mason, PhD2, Marek Steslicki5, Szymon Gburek5, Janusz Sylwester5, Craig E DeForest6, Richard Schwartz7 and Geoff Crowley8, (1)Southwest Research Institute, Boulder, CO, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Naval Research Laboratory, Washington, DC, United States, (4)Laboratory for Atmospheric and Space Physics, Boulder, United States, (5)Space Research Centre, Polish Academy of Sciences, Wrocław, Poland, (6)Southwest Research Institute Boulder, Boulder, CO, United States, (7)NASA GSFC, Solar Physics Lab, Greenbelt, MD, United States, (8)Orion Space Solutions, Louisville, United States
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