SH007
Frontier Discovery from the Whole Heliosphere and Planetary Interactions (WHPI) Initiative

Session ID#: 82608

Session Description:
Profound progress is possible when community-wide cooperation and coordination is accomplished, perhaps best illustrated recently by the remarkable feat of imaging a black hole for the first time by coordinating the power of eight major radio observatories on four continents and over 200 astronomers. Similarly, the the Whole Heliosphere and Planetary Interactions (WHPI) initiative is a pioneering effort to coordinate global, community-wide observation and modeling efforts to characterize the 3-dimensional interconnected solar-heliospheric-planetary system, carrying to the current solar minimum the heritage of the Whole Sun Month (1996) and Whole Heliosphere Interval (2008). This session will feature efforts and results to observe the full breadth of Sun-Earth-planets and to comprehensively map the solar-minimum heliosphere via state-of-the-art models. We seek abstracts from individuals and teams of researchers to support WHPI. Goals are to reveal WHPI progress, bring together the WHPI community for active discussions, and reveal best practices for community-wide coordination efforts.
Co-Organized:
  • P - Planetary Sciences
  • SA - SPA-Aeronomy
  • SM - SPA-Magnetospheric Physics
Index Terms:

6299 General or miscellaneous [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
7536 Solar activity cycle [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7999 General or miscellaneous [SPACE WEATHER]

Primary Convener:  Ryan Michael McGranaghan, Atmospheric and Space Technology Research Associates (ASTRA), Louisville, CO, United States
Conveners:  Giuliana de Toma, NCAR, Boulder, CO, United States, Gina A DiBraccio, University of Michigan, Ann Arbor, MI, United States and Sarah E Gibson, NCAR, HAO, Boulder, CO, United States
Primary Liaison:  Giuliana de Toma, NCAR, Boulder, CO, United States
 
Weakening Solar Polar Fields, the Terrestrial Magnetosphere and the Forthcoming Solar Cycle (515214)
Janardhan Padmanabhan, Physical Research Laboratory, Ahmedabad, India and Susanta Kumar Bisoi, National Astronomical Observatories, Chinese Academy of Sciences, Key Laboratory of Solar Activity, Beijing, China
 
Solar Spectral Irradiance during WHPI and comparison to WHI and WSM (542032)
Martin A Snow1, Stephane Beland2, Erik C Richard3, Thomas N Woods3, Francis Epavier4 and Philip Chamberlin2, (1)University of Colorado at Boulder, Boulder, CO, United States, (2)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (3)University of Colorado Boulder, Boulder, CO, United States, (4)Univ Colorado, Boulder, CO, United States
 
Total Electron Content and Ionospheric Scintillation Measurements during the Total Solar Eclipse of July 2, 2019 (548646)
Lucas Eduardo Tijerina1, Daniel Nigro1, Jose Nicolas Gachancipa1, Julian Andres Herrera1, Chintan Thakrar1, Pralay Raj Vaggu1, Michael Fitzpatrick1, Danayit Mekonnen1, Kshitija Deshpande1, Alan Liu1 and Pablo Rubén Muñoz2, (1)Embry-Riddle Aeronautical University, Department of Physical Sciences, Daytona Beach, FL, United States, (2)University of La Serena, Department of Physics and Astronomy, La Serena, Chile
 
From Aleph to TAV: SORCE/SIM Recalibration Using TSIS (552493)
Joel Matthew Tibbetts, Steven Victor Penton, Stephane Beland, Jerald William Harder, Martin A Snow and Thomas N Woods, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
 
Perturbation of the Ionosphere-Thermosphere System due to the July 2, 2019 Total Solar Eclipse as Observed by the Global-scale Observations of the Limb and Disk (GOLD) Mission (554919)
Saurav Aryal1, Tong Dang2, Jiuhou Lei2, Huixin Liu3, Geonhwa Jee4, Wenbin Wang5, Alan Geoffrey Burns5, Stanley C Solomon5, J. Scott Evans6, Victoir Veibell6, Andrey Krywonos7, William E McClintock1, Richard Eastes1 and the GOLD Science team, (1)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)University of Science and Technology of China, Hefei, China, (3)Kyushu University, Fukuoka, Japan, (4)Korea Polar Research Institute, Division of Polar Climate Sciences, Incheon, South Korea, (5)NCAR, HAO, Boulder, CO, United States, (6)Computational Physics Inc. Springfield, Springfield, VA, United States, (7)UCF-Florida Space Institute, Orlando, FL, United States
 
Modulation of the Galactic Cosmic Radiation through Solar Cycle 25: Predictions in the Case of a Modern Secular Minimum Condition (559088)
Fatemeh Rahmanifard1, Wouter Christiaan de Wet2, Nathan Schwadron2, Mathew James Owens3, Andrew Jordan1, Jody Keith Wilson1, Colin Joyce4, Charles W Smith5, Harlan E. Spence2 and Larry Townsend6, (1)University of New Hampshire Main Campus, Space Science Center, Durham, NH, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Uinversity of Reading, Reading, United Kingdom, (4)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States, (5)University of New Hampshire Main Campus, Durham, NH, United States, (6)Arlington, MA, United States
 
Following the evolution of coronal mass ejections across the heliosphere (578256)
Erika Palmerio1, Olivier G Witasse2, Teresa Nieves-Chinchilla3, David Barnes4, Marilena Mierla5, Andreas J Weiss6, Christian Moestl7, Andrei Zhukov8, Lan Jian3, Beatriz Sanchez-Cano9, Luciano Rodriguez5, Jingnan Guo10, Elias Roussos11, Adam Masters12, Gabrielle Provan13, Alexey Isavnin14, Patrick J Lowrance15, Lucile Turc16 and K Emilia J Kilpua1, (1)University of Helsinki, Helsinki, Finland, (2)European Space Agency, Noordwijk, Netherlands, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (5)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (6)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (7)Institute of Physics, University of Graz, Graz, Austria, (8)Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia, (9)University of Leicester, Leicester, LE1, United Kingdom, (10)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (11)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (12)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan, (13)University of Leicester, Leicester, United Kingdom, (14)Rays of Space Oy, Vantaa, Finland, (15)IPAC–Spitzer, California Institute of Technology, Pasadena, CA, United States, (16)LPP - CNRS - Ecole polytechnique - UPMC, Palaiseau, France
 
Utilizing the Madrigal database in the WHPI Initiative (Invited) (584535)
Anthea Coster and William E Rideout, MIT Haystack Observatory, Westford, MA, United States
 
WHPI Hα “McIntosh” Carrington Maps (586832)
Ian McDonald Hewins1, Sarah E Gibson2, David F Webb3, Thomas A Kuchar3, Robert McFadden4 and Barbara A Emery-Geiger5, (1)Organization Not Listed, Washington, DC, United States, (2)NCAR, HAO, Boulder, CO, United States, (3)Boston College, ISR, Chestnut Hill, MA, United States, (4)High Altitude Observatory, Boulder, CO, United States, (5)ISR, Boston College at HAO/NCAR, Boulder, CO, United States
 
Observations of Space Weather at Mars (613940)
Dave A Brain1, Christina O Lee2,3, Gina A DiBraccio4,5, Jared R Espley6, Jasper S Halekas7, Andrea C. G. Hughes8, Sonal Jain9, Nicholas McCord Schneider10, Edward Thiemann9, Janet G Luhmann11 and Bruce Martin Jakosky12, (1)University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (2)Boston College, Institute for Scientific Research, Chestnut Hill, MA, United States, (3)Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States, (4)University of Michigan, Ann Arbor, MI, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)Goddard Space Flight Center, Greenbelt, MD, United States, (7)University of Iowa, Department of Physics and Astronomy, Iowa City, IA, United States, (8)Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (10)Univ Colorado, Boulder, CO, United States, (11)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (12)University of Colorado Boulder, Boulder, CO, UNITED STATES
 
Combining Broadband Irradiance Measurements and Plasma Temperature Approximations to Generate Solar EUV Spectra (629308)
Vicki Knoer, Boulder, CO, United States, Edward Thiemann, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Francis Epavier, Univ Colorado, Boulder, CO, United States, Phillip C Chamberlin, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Thomas N Woods, University of Colorado Boulder, LASP, Boulder, CO, United States
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