SH41E:
Space Weather Research and Forecasting: Building Tomorrow's Space Weather Architectures Posters


Submit an Abstract to this Session


Session ID#: 49222

Session Description:
We still find that society is ever-more reliant on technologies/energy supplies susceptible to interruption/damage from space weather (SW) (communications/transport, GNSS-positioning/timing, power, etc.). As a result, several new infrastructures, missions, and models are being developed to improve forecasting capabilities, our understanding of the impacts, and to engineer in better mitigation solutions.

This is fourth incarnation of the session (since 2015) where the focus now specifically turns to new ideas about future space-/ground-based SW architectures. Multiple ongoing international studies are scoping the options for sustained/improved SW observations. New observing locations (e.g. L5) as well as advanced concepts based on small satellites and splitting larger missions into smaller sub-elements (fractionation) are being considered in these studies.

We solicit contributions of: ideas/discussions regarding sustainable SW observations/architectures; how small satellites can be used to supplement SW architectures; whether GOES-SWFO-L5 provides the needed observations/sustainability; and what new technologies challenge the past ways of undertaking SW research/operations.

Primary Convener:  Mario Mark Bisi, STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom
Conveners:  Antti A Pulkkinen, NASA/GSFC, Greenbelt, MD, United States, Mark Gibbs, Met Office, Exeter, United Kingdom and Brent Gordon, NOAA Space Weather Prediction Center, Boulder, CO, United States
Primary Liaison:  Mario Mark Bisi, United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
Chairs:  Brent Gordon, NOAA Space Weather Prediction Center, Boulder, CO, United States and Mark Gibbs, Met Office, Exeter, United Kingdom
OSPA Liaison:  Antti A Pulkkinen, NASA/GSFC, Greenbelt, MD, United States
Co-Organized with:
SPA-Solar and Heliospheric Physics, and SPA-Magnetospheric Physics

Cross-Listed:
  • NH - Natural Hazards
  • SA - SPA-Aeronomy
  • SI - Societal Impacts and Policy Sciences

Proposed Co-Organized Session with:
  • SM - SPA-Magnetospheric Physics
Index Terms:

4305 Space weather [NATURAL HAZARDS]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7924 Forecasting [SPACE WEATHER]
7999 General or miscellaneous [SPACE WEATHER]

Abstracts Submitted to this Session:

Latest Community Coordinated Modeling Center (CCMC) services and innovative tools supporting the space weather research and operational communities. (433766)
Anne Michelle M Mendoza1, Maria M Kuznetsova2, Leila M Mays3, Lutz Rastaetter1, Anna Chulaki4, Peter J MacNeice5, Ja Soon Shim6, Aleksandre Taktakishvili7, Yaireska M Collado-Vega8, Chui Weigand9, Richard Mullinix10, Tina Tsui8, Asher D Pembroke11 and Community Coordinated Modeling Center (CCMC), (1)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, MD, United States, (2)NASA/GSFC, Community Coordinated Modeling Center, Greenbelt, United States, (3)NASA/GSFC, Heliophysics, Greenbelt, United States, (4)NASA GSFC/CUA, Greenbelt, United States, (5)NASA Goddard SFC, Greenbelt, United States, (6)Catholic University of America, Washington, DC, United States, (7)Catholic University of America, Washington, United States, (8)NASA GSFC, Greenbelt, United States, (9)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (10)Community Coordinated Modeling Center, NASA Goddard Space Flight Center, Greenbelt, United States, (11)Predictive Science Inc., San Diego, CA, United States
Space Very Low Frequency Solar Radio Imaging Array (431725)
Yihua Yan1, Linjie Chen2, Wei Wang2, Guangyou Fang3 and Baolin Tan2, (1)National Astronomical Observatories, Beijing, China, (2)National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China, (3)Institute of Electronics, Beijing, China
The Prediction of Bz Fields Using the CSSS Model and UCSD IPS Tomography (440459)
Hsiu-Shan Yu1, Bernard V Jackson2,3, Andrew Buffington2, P. Paul Hick2 and Munetoshi Tokumaru4, (1)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (2)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (3)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (4)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan
LOFAR4SpaceWeather (LOFAR4SW) – Increasing European Space-Weather Capability with Europe’s Largest Radio Telescope: Steps Toward the Preliminary Design Review (PDR) (414788)
Mario Mark Bisi1, Rene Vermeulen2, Richard Andrew Fallows2, Nicole Vilmer3, Hanna Rothkaehl4, Joris Verbiest5, Peter Gallagher6, Michael Olberg7, Eoin Carley8, Maaijke Mevius2 and Stuart Charles Robertson9, (1)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (2)ASTRON, The Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (3)Observatoire Paris, Meudon, France, (4)Space Research Centre, PAS, Warsaw, Poland, (5)Bielefeld University, Bielefeld, Germany, (6)Trinity College Dublin, Dublin, Ireland, (7)Chalmers University of Technology, Gothenburg, Sweden, (8)Dublin Institute for Advanced Studies, Dublin, Ireland, (9)United Kingdom Research and Innovation – Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Harwell Campus, United Kingdom
Observations of a Coronal Mass Ejection using Interplanetary Scintillation (IPS) and Comparison with Numerical Models (417030)
Oyuki Chang, UKRI STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, Ricardo F. González, Instituto de Radioastronomía y Astrofísica, UNAM, Morelia, Michoacán, Mexico, Mario Mark Bisi, United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom and Richard Andrew Fallows, ASTRON, The Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands
Radio-continuum Emission from the Interaction of a Coronal Mass Ejection with the Solar Wind (468552)
Ricardo F. González, National Autonomous University of Mexico, Ciudad DE Armería, Mexico, Daniela Montes Doria Jr., Antioquia University, Astronomy, Medellin, Colombia and Jose Carlos Olvera Meneses Jr, Universidad Autonoma del Estado de Hidalgo, Mathematics, Hidalgo, Mexico
The UCSD Iterative Interplanetary Scintillation (IPS) Analysis Using an ENLIL 3-D MHD Model Kernel in Near Real Time (429021)
Bernard V Jackson1, Hsiu-Shan Yu2, P. Paul Hick3, Andrew Buffington3, Dusan Odstrcil4, Munetoshi Tokumaru5 and Mario Mark Bisi6, (1)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (2)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (3)University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (4)George Mason University Fairfax, Fairfax, VA, United States, (5)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (6)United Kingdom Research and Innovation - Science & Technology Facilities Council, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
Nowcast of Kp and high cadence global geomagnetic indices (407727)
Dr. Guram Kervalishvili1, Juergen Matzka1, Claudia Stolle1 and Jan Rauberg2, (1)GFZ German Research Centre for Geosciences, Potsdam, Germany, (2)GFZ Helmholtz Centre for Geosciences, 2.3 Geomagnetism, Potsdam, Germany
WSA-ENLIL+Cone Modeling of CMEs in 2010-2011 Using Multipoint Spacecraft Observations (448247)
Lan Jian1, Dusan Odstrcil1,2, M. Leila Mays3, RyunYoung Kwon2,4 and Sachiko Akiyama5,6, (1)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (2)George Mason University Fairfax, Fairfax, VA, United States, (3)NASA Goddard Space Flight Center, Community Coordinated Modeling Center, Greenbelt, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, VA, United States, (5)Catholic University of America, Washington, United States, (6)NASA Goddard Space Flight Center, Greenbelt, United States
Improving MAG4’s Forecasting of Drivers of Severe Space Weather (415103)
Megan Anne Fisher, College of Wooster, Wooster, OH, United States, David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States, Ronald Lee Moore, NASA MSFC, Huntsville, United States and Sanjiv K. Tiwari, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States
Providing Long-term Measurements of 5 - 50 MeV/nucleon Proton and Helium Intensities – A new Data Product for SOHO/EPHIN (377295)
Patrick Kühl1, Bernd Heber2 and Lars Berger1, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Kiel, Kiel, Germany
Heavy Ion Composition and Flux Measurements as a New, Sustainable Window on Space Weather: Observations From the GOES-16 Energetic Heavy Ion Sensor (EHIS) (433467)
James J Connell, University of New Hampshire, Physics, Durham, NH, United States and Clifford Lopate, University of New Hampshire Main Campus, Durham, NH, United States
The Solar Polar Constellation (SPOC) Mission: Combining Operational Full-Sun Magnetic Field Measurements with Polar Exploration (438641)
Thomas E Berger1, Nicole A Duncan2, Daniel N Baker3, Jeffrey P Thayer4, Steven R Cranmer5, Christopher K Pankratz3, Neal E Hurlburt6 and Natasha Bosanac7, (1)University of Colorado, Space Weather Technology, Research, and Education Center, Boulder, United States, (2)Ball Aerospace, Boulder, CO, United States, (3)University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, United States, (4)University of Colorado at Boulder, Smead Aerospace Engineering Sciences, Boulder, United States, (5)University of Colorado at Boulder, APS, Boulder, CO, United States, (6)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (7)University of Colorado, Dept. of Aerospace Engineering Sciences, Boulder, CO, United States
A SOlar Dynamo Amplitude (SODA) Prediction of Approximately 140 for Cycle 25's F10.7 Radio Flux (375006)
Joel Getchius, University of Houston Clear Lake, Houston, TX, United States, William Dean Pesnell, NASA / GSFC, Greenbelt, United States and Kenneth H. Schatten, a.i. solutions, Inc., Lanham, MD, United States
Response of Schumann resonance parameters to intense solar activity (434173)
Akihiro Ikeda, Kagoshima National College of Technology, Kagoshima, Japan, Teiji Uozumi, Kyushu University, International Center for Space Weather Science and Education, Fukuoka, Japan, Akimasa Yoshikawa, Kyushu University, Department of Earth and Planetary Sciences, Fukuoka, Japan, Akiko Fujimoto, Kyushu Institute of Technology, Department of Artificial Intelligence, Izuka, Japan and Shuji Abe, Kyushu University, International Research Center for Space and Planetary Environmental Science, Fukuoka, Japan

See more of: SPA-Solar and Heliospheric Physics