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

Session ID#: 2941

Tuesday, 16 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  William Dean Pesnell, NASA / GSFC, Greenbelt, United States and Bernard V Jackson, University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States
Primary Convener:  Scott William McIntosh, High Altitude Observatory, Boulder, United States
Co-conveners:  William Dean Pesnell, NASA / GSFC, Greenbelt, United States, Mario Mark Bisi, STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom and Bernard V Jackson, University of California San Diego, Astronomy and Astrophysics, La Jolla, CA, United States
OSPA Liaison:  Scott William McIntosh, High Altitude Observatory, Boulder, United States
Index Terms:

7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7536 Solar activity cycle [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7938 Impacts on humans [SPACE WEATHER]
Virtual Option?: No

Abstracts Submitted to this Session:

 
Grand Minima: Is The Sun Going To Sleep? (26995)
Scott William McIntosh, High Altitude Observatory, Boulder, United States and Robert James Leamon, NASA Headquarters, Washington, MD, United States
 
Pushing the Envelope of Extreme Space Weather (8902)
William Dean Pesnell, NASA / GSFC, Greenbelt, United States
 
Computing Solar EUV Irradiance Variability (21559)
Harry P Warren, Naval Research Laboratory, Washington, DC, United States
 
Sorce Observations of Solar Cycles 23 and 24 – What's New? What's Next? (9542)
Robert F Cahalan, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Greg Kopp, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, United States, Peter Pilewskie, University of Colorado at Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, Erik C Richard, LASP, University of Colorado, Boulder, United States and Thomas N Woods, University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
 
Time-Dependent Coupling of Lfm-Helio and MAS Models for CME Propagation (10995)
John Lyon, Dartmouth College, Hanover, NH, United States, Viacheslav G Merkin, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Roberto Lionello, Predictive Science Inc., San Diego, United States, Jon Linker, Predictive Science Inc., San Diego, CA, United States and Nour E 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 (4027)
O Kenneth Moe, Space Environment Technologies, Pacific Palisades, CA, United States and Qian Wu, NCAR, Boulder, United States
 
Speed of CMEs and the magnetic non-potentiality of their source active regions (25157)
Navdeep Kaur Panesar, NASA Marshall Space Flight Center, Huntsville, AL, United States, David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States, Ronald Lee Moore, NASA Marshall Space Flight Center, Huntsville, United States and P. Venkatakrishnan, Udaipur Solar Observatory, Udaipur, India
 
A COSPAR/ILWS roadmap towards advanced space weather science to protect society's technological infrastructure (20800)
Karel Schrijver, Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States, Kirsti Kauristie, Finnish Meteorological Institute, Helsinki, Finland and COSPAR/ILWS Roadmap Team
 
A space weather information service based upon remote and in-situ measurements of coronal mass ejections heading for Earth (21030)
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 Réville, Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, 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 (11037)
Ward Manchester, Bart van der Holst and Igor Sokolov, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
A magnetically-driven model of flux-rope expansion from the Sun to 1AU in order to compute Bz at 1AU. (2966)
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 (21761)
Hong Xie, NASA/GSFC, Greenbelt, United States, Nat Gopalswamy, NASA Goddard SFC, Greenbelt, United States, Seiji Yashiro, Catholic University of America, Washington, DC, United States and Sachiko Akiyama, NASA Goddard Space Flight Center, Greenbelt, United States
 
Probabilistic Forecasting Analysis of Geomagnetic Indices for IMF Bs-events (12554)
Xiangyun Zhang, University of Michigan, Ann Arbor, MI, United States and Mark B Moldwin, University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
 
Predicting the high-speed-stream caused Bs events using the Current Sheet Source Surface Model (22316)
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 (13926)
Alisson Dal Lago1, Tardelli Ronan Coelho Stekel1, Carlos Roberto Braga1, Luis Eduardo A Vieira2, Laura Antonia Balmaceda1, Rashmi Rawat1, Ezequiel Echer1 and Walter D Gonzalez1, (1)INPE National Institute for Space Research, Sao Jose dos Campos, Brazil, (2)INPE National Institute for Space Research, Space Geophysics Division, Sao Jose dos Campos, Brazil
 
Faraday Rotation (FR) and Interplanetary Scintillation (IPS) Case Studies Using the LOw Frequency ARray (LOFAR) (29386)
Mario Mark Bisi1, Richard Andrew Fallows2, C Sobey3, T Eftekhari3,4, Elizabeth A Jensen5, Bernard V Jackson6, Hsiu-Shan Yu7, Daniel J Gershman8,9, Jim M Raines10 and Dusan Odstrcil11,12, (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)ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (4)University of New Mexico Main Campus, Albuquerque, NM, United States, (5)Planetary Science Institute Tucson, Tucson, United States, (6)University of California, San Diego, Astronomy and Astrophysics, La Jolla, CA, United States, (7)University of California San Diego, Center for Astrophysics and Space Science, La Jolla, CA, United States, (8)NASA Goddard Space Flight Center, Greenbelt, United States, (9)University of Michigan Ann Arbor, Department of Atmospheric, Oceanic and Space Sciences, Ann Arbor, MI, United States, (10)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (11)George Mason University Fairfax, Fairfax, VA, United States, (12)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States
 
Using IPS Magnetic Modeling to Determine Bz (17346)
Bernard V Jackson1, Hsiu-Shan Yu2, P. Paul Hick3, Andrew Buffington3, Julio Cesar Mejia-Ambriz4, Mario Mark Bisi5 and Munetoshi Tokumaru6, (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)University of California San Diego, La Jolla, CA, United States, (5)STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom, (6)Nagoya University, Nagoya, Japan