SH21C:
Sun-Earth Connection: A Mid-Course Correction, and Observations and Modeling of Bz I Posters

Tuesday, 16 December 2014: 8:00 AM-12:20 PM
Chairs:  William Dean Pesnell, NASA / GSFC, Greenbelt, MD, United States and Bernard V Jackson, Univ California San Diego, La Jolla, CA, United States
Primary Conveners:  Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States
Co-conveners:  William Dean Pesnell, NASA / GSFC, Greenbelt, MD, United States, Mario Mark Bisi, Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom and Bernard V Jackson, Univ California San Diego, La Jolla, CA, United States
OSPA Liaisons:  Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States

Abstracts Submitted to this Session:

 
Grand Minima: Is The Sun Going To Sleep?
Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States and Robert James Leamon, NASA Headquarters, Washington, DC, United States
 
Pushing the Envelope of Extreme Space Weather
William Dean Pesnell, NASA / GSFC, Greenbelt, MD, United States
 
Computing Solar EUV Irradiance Variability
Harry P Warren, Naval Research Lab DC, Washington, DC, United States
 
Sorce Observations of Solar Cycles 23 and 24 – What's New? What's Next?
Robert F Cahalan1, Greg Kopp2, Peter Pilewskie3, Erik C Richard2 and Thomas N Woods2, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Univ Colorado, Boulder, CO, United States, (3)University of Colorado at Boulder, Boulder, CO, United States
 
Time-Dependent Coupling of Lfm-Helio and MAS Models for CME Propagation
John Lyon, Dartmouth College, Hanover, NH, United States, Viacheslav G Merkin, The Johns Hopkins University, Laurel, MD, United States, Roberto Lionello, Predictive Science Incorporate, San Diego, CA, United States, Jon Linker, Predictive Science Inc., San Diego, CA, United States and Nour-Eddine Raouafi, Johns Hopkins University, Baltimore, MD, United States
 
Hiwind Balloon Fabry-Perot Interferometer Measurements Show the Importance of the Solar Wind Influence on Thermospheric Density and Wind Models at Quiet Times
O Kenneth Moe, Space Environment Technologies, Hawthorne, CA, United States and Qian Wu, NCAR, Boulder, CO, United States
 
Speed of CMEs and the magnetic non-potentiality of their source active regions
Sanjiv K. Tiwari1, David Allen Falconer2, Ronald L Moore1 and P. Venkatakrishnan3, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)National Space Science and Technology Center, Huntsville, AL, United States, (3)Udaipur Solar Observatory, Udaipur, India
 
A COSPAR/ILWS roadmap towards advanced space weather science to protect society's technological infrastructure
Karel Schrijver, Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States and Kirsti Kauristie, Finnish Meteorological Inst, Helsinki, Finland
 
A space weather information service based upon remote and in-situ measurements of coronal mass ejections heading for Earth
Birgit Ritter, German Aerospace Center DLR Cologne, Cologne, Germany, Oliver Andreas Hartkorn, University of Cologne, Cologne, Germany, Arjan J. H. Meskers, Delft University of Technology, Faculty of Mechanical Engineering, Delft, Netherlands, Oscar Miles, University of Southampton, Faculty of Applied Sciences and Engineering, Southampton, United Kingdom, Michael Russwurm, Vienna University of Technology, Vienna, Austria, Steven Scully, National University of Ireland Maynooth, Department of Experimental Physics, Kildare, United Kingdom, Andres Roldan, University of Granada, Faculty of Sciences, Granada, Spain, Peter Juestel, University of Stuttgart, Stuttgart, Germany, Victor Reville, CEA/Irfu Paris Diderot University CNRS/INSU, AIM Paris-Saclay Laboratory, Paris, France, Sorina Lupu, Politehnica University of Bucharest, Faculty of Electronics, Bucharest, Romania and Alexis Ruffenach, IRAP, Toulouse, France
 
Predicting ICME Magnetic Fields with a Numerical Flux Rope Model
Ward Manchester, Bart van der Holst and Igor Sokolov, University of Michigan, Ann Arbor, MI, United States
 
A magnetically-driven model of flux-rope expansion from the Sun to 1AU in order to compute Bz at 1AU.
Valbona Kunkel, George Mason University Fairfax, Fairfax, VA, United States, Alexis P Rouillard, IRAP, Toulouse, France and Anthony Bourdelle, University Paul Sabatier Toulouse III, Toulouse Cedex 09, France
 
Estimation of Reconnection Flux using Post-eruption Arcades and Prediction of Bz at Earth
Hong Xie, NASA/GSFC, Greenbelt, MD, United States, Nat Gopalswamy, NASA Goddard SFC, Greenbelt, MD, United States, Seiji Yashiro, Catholic University of America, Washington, DC, United States and Sachiko Akiyama, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Probabilistic Forecasting Analysis of Geomagnetic Indices for IMF Bs-events
Xiangyun Zhang and Mark Moldwin, University of Michigan, Ann Arbor, MI, United States
 
Predicting the high-speed-stream caused Bs events using the Current Sheet Source Surface Model
Bala Poduval, Space Science Institute Boulder, Boulder, CO, United States and Xuepu Zhao, Stanford University, HEPL, Stanford, CA, United States
 
Forecasting Dst index using CME expansion speed
Alisson Dal Lago, Tardelli Ronan Coelho Stekel, Carlos Roberto Braga, Luis Eduardo A Vieira, Laura Antonia Balmaceda, Rashmi Rawat, Ezequiel Echer and Walter D Gonzalez, INPE National Institute for Space Research, Sao Jose dos Campos, Brazil
 
Faraday Rotation (FR) and Interplanetary Scintillation (IPS) Case Studies Using the LOw Frequency ARray (LOFAR)
Mario Mark Bisi1, R A Fallows2, C Sobey2, T Eftekhari2,3, Elizabeth A Jensen4, Bernard V Jackson5, Hsiu-Shan Yu5, Daniel J Gershman6,7, Jim M Raines7 and Dusan Odstrcil6,8, (1)Rutherford Appleton Lab, RAL Space, Harwell Oxford, Didcot, United Kingdom, (2)ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (3)University of New Mexico Main Campus, Albuquerque, NM, United States, (4)Planetary Science Institute Tucson, Tucson, AZ, United States, (5)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (6)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (7)University of Michigan Ann Arbor, Department of Atmospheric, Oceanic and Space Sciences, Ann Arbor, MI, United States, (8)George Mason University Fairfax, School of Physics, Astronomy, and Computational Sciences, Fairfax, VA, United States
 
Using IPS Magnetic Modeling to Determine Bz
Bernard V Jackson1, Hsiu-Shan Yu2, P. Paul Hick2, Andrew Buffington2, Julio Cesar Mejia-Ambriz2, Mario Mark Bisi3 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, La Jolla, CA, United States, (3)Rutherford Appleton Laboratory, Didcot, OX11, United Kingdom, (4)Nagoya University, Nagoya, Japan