SH007
Data Mining For Science of the Sun-Earth Connection

Session ID#: 159074

Session Description:
Direct measurements by in situ instruments are detailed and precise measurements of physical observables, which cannot be gained from remote observations.  Remote sensing observations, in turn, provide large-scale context, which is absent from the in situ data taken at one point in space.  Therefore, to understand the Sun-Earth system, we need to effectively establish a link between in situ measurements and remote observations by characterizing structure and plasma properties of the Sun/corona/heliosphere through the improved use of increasingly diverse data sets and a profusion of data analysis and processing techniques.  The main purpose of this session is to discuss the various observations, analysis tools and models that are essential to extract information about the Sun-Earth connection as a single system.  We encourage submissions on current and/or future efforts and/or challenges for observations, analysis/processing tools, models and theory that aim to decipher the physics of the Sun-Earth connection.
Index Terms:

2169 Solar wind sources [INTERPLANETARY PHYSICS]
2784 Solar wind/magnetosphere interactions [MAGNETOSPHERIC PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7594 Instruments and techniques [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Primary Convener:  Nathalia Alzate, NASA Goddard Space Flight Center / ADNET Systems, Inc., Greenbelt, United States; ADNET Systems Inc., Greenbelt, MD, United States
Conveners:  Daniel B Seaton, Southwest Research Institute, Boulder, United States and Simone Di Matteo, Catholic University of America, Physics Department, Washington, United States; NASA Goddard Space Flight Center / Catholic U. of America, Greenbelt, United States
 
Synthetic solar wind generator (1055076)
Enrico Camporeale, University of Colorado/CIRES, Boulder, CO, United States and Andong Hu, University of Colorado at Boulder, Boulder, United States
 
Validation of Image Based Method for Assessing Coronal Magnetic Field Models (1093358)
Christopher Rura1,2, Vadim Uritsky1,2, Shaela I Jones1,2, Charles Nickolos Arge2 and Nathalia Alzate2,3, (1)Catholic University of America, Washington, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)ADNET Systems Inc., Greenbelt, United States
 
Resolving CME Characteristics with Polarized PUNCH Data (1096041)
Matthew John West1, James Marcus Hughes2, Bryce Walbridge3, Daniel B Seaton4, Craig DeForest5, Chris Lowder5, Sarah E Gibson6 and Anna V Malanushenko7, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute Boulder, Boulder, CO, United States, (3)Calvin University, Zeeland, United States, (4)Southwest Research Institute, Boulder, United States, (5)Southwest Research Institute, Boulder, CO, United States, (6)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (7)LMSAL, Palo Alto, CA, United States
 
The transmission of ULF waves from the solar wind to the magnetosphere: an analysis of some critical aspects. (1106439)
Dario Recchiuti, University of Trento, Trento, Italy, Umberto Villante, University of L'Aquila, L'Aquila, Italy and Simone Di Matteo, Catholic University of America, Washington, United States
 
Magnetic Field Reconnection as the Source of the Solar wind (Invited) (1116448)
Nour E. Raouafi1, Guillermo A Stenborg2, Daniel B Seaton3, Haimin Wang4, Jiasheng Wang5, Craig DeForest6, Stuart Bale7, James Frederick Drake8, Timothy Simon Horbury9, Vadim Uritsky10, Judith T Karpen11, Sofiane Bourouaine2, Marco C M Velli12, Justin Christophe Kasper13, Pankaj Kumar14, C Richard DeVore15, Lakshmi Pradeep Chitta16 and Tai Phan17, (1)Johns Hopkins University, Baltimore, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (3)Southwest Research Institute, Boulder, United States, (4)New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States, (5)State Key Laboratory of Biogeology and Environmental Geology, Wuhan, China, (6)Southwest Research Institute, Boulder, CO, United States, (7)University of California, Berkeley, Berkeley, CA, United States, (8)University of Maryland College Park, College Park, MD, United States, (9)Imperial College London, Department of Physics, London, SW7, United Kingdom, (10)Catholic University of America, Washington, United States, (11)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (12)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (13)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (14)American University at NASA GSFC, Greenbelt, MD, United States, (15)NASA Goddard Space Flight Center, Greenbelt, United States, (16)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (17)University of California Berkeley, Berkeley, CA, United States
 
A Revised Database of CME Characteristics from In-situ and Remote Observations (1149193)
Simone Chierichini1,2, Teresa Barata3, Enrico Camporeale4, Dario Del Moro2, Giancarlo De Gasperis2, Robertus Erdelyi1, João Manuel Fernandes5, Raffaello Foldes6,7, Gregoire Francisco2,8, Luca Giovannelli2, Ronish Mugatwala1,2, Gianluca Napoletano2,9, Ajay Tiwari10 and Jannis Teunissen10, (1)University of Sheffield, School of Mathematics and Statistics, Sheffield, United Kingdom, (2)University of Rome Tor Vergata, Physics, Rome, Italy, (3)University of Coimbra, IA-UC, Faculty of Sciences and Technologies, Coimbra, Portugal, (4)University of Colorado, Boulder, United States, (5)University of Coimbra, CITEUC, Coimbra, Portugal, (6)University of L'Aquila, Department of Physical and Chemical Sciences, L'Aquila, Italy, (7)École Centrale de Lyon, Laboratoire de Mécanique des Fluides et Acoustique, Lyon, France, (8)University of Coimbra, Coimbra, Portugal, (9)University of L'Aquila, L'Aquila, Italy, (10)Centrum Wiskunde & Informatica, Amsterdam, Netherlands
 
Radiation Data Portal: Enhancing Data Discoverability and Analysis for Understanding Space Radiation in Earth Environment (1157001)
Viacheslav M Sadykov1, Zachary M Watkins2, Dustin Kempton1, Xiaochun He2, W Kent Tobiska3, Christopher J Mertens4, Shubha Ranjan5, Irina Kitiashvili6, Ryan Spaulding7 and Glenn Deardorff8, (1)Georgia State University, Atlanta, GA, United States, (2)Georgia State University, Atlanta, United States, (3)Space Environment Technologies, Pacific Palisades, CA, United States, (4)NASA Langley Research Ctr, Hampton, VA, United States, (5)NASA Ames Research Center, Moffett Field, United States, (6)NASA Ames Research Center, Moffett Field, CA, United States, (7)NASA Ames Research Center, Boulder, CO, United States, (8)NASA Ames Research Center, NAS, Moffett Field, United States
 
Pathfinding Solar Tomography for Future Missions via Model Data Reconstruction (1170650)
James Marcus Hughes1, F Auchere2, Amir Caspi3, Gabriel Pelouze4, Joseph Plowman3, Daniel B Seaton5 and Matthew John West3, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France, (3)Southwest Research Institute, Boulder, CO, United States, (4)Université Paris-Saclay, Orsay, France, (5)Southwest Research Institute, Boulder, United States
 
Single and Multiple Vantage Point 3D Coronal Reconstruction with the CROBAR Method (1176020)
Joseph Plowman1, Amir Caspi1, Don Hassler1, James Marcus Hughes2, Daniel B Seaton3 and Matthew John West1, (1)Southwest Research Institute, Boulder, CO, United States, (2)Southwest Research Institute Boulder, Boulder, United States, (3)Southwest Research Institute, Boulder, United States
 
What Lurks Below the Noise Floor (1177814)
Craig E. DeForest, Southwest Research Institute Boulder, Boulder, CO, United States, Daniel B Seaton, Southwest Research Institute, Boulder, United States, Matthew John West, Royal Observatory of Belgium, Brussels, Belgium and Chris Lowder, Southwest Research Institute, Boulder, CO, United States
 
Optimized Coronal Magnetic Field Models Using STEREO COR-1 Images, with Solar Wind Speed and IMF Prediction Comparisons (1178247)
Shaela I Jones1,2, Vadim M Uritsky1,2, Nathalia Alzate3, Christopher Rura2, Charles Nickolos Arge4 and James H Staeben5, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, United States, (3)ADNET Systems Inc., Greenbelt, United States, (4)NASA Goddard Space Flight Center, Greenbelt, United States, (5)University of Virginia, Charlottesville, United States
 
Visualizing Enlil and EUHFORIA CME Propagation Models using an Accessible Interactive 3-Dimensional Data Visualization Tool (1185429)
Christopher K Pankratz, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, Greg Lucas, Univ of Colorado, Boulder, United States, Jenny Knuth, University of Colorado Boulder, Boulder, CO, United States, Dusan Odstrcil, George Mason University, Fairfax, VA, United States and Thomas E Berger, University of Colorado at Boulder, Space Weather Technology, Research, and Education Center, Boulder, United States
 
SynCOM: A dynamic model for flow tracking algorithms (1196812)
Valmir Moraes Filho, Catholic University of America, Washington, DC, United States, Vadim Uritsky, Catholic University of America, Washington, United States, Barbara J Thompson, NASA/GSFC, Greenbelt, MD, United States and Craig DeForest, Southwest Research Institute, Boulder, CO, United States
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