SA44A:
Advances in Radio Frequency Propagation Modeling and Applications II

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Session ID#: 18249

Session Description:
Radio frequency propagation modeling is an integral part of a wide variety of scientific studies and technological applications. Many models and applications consider the effects of ionospheric refraction, magneto-ionic splitting, plasma and neutral collisions, scintillation, traveling ionospheric disturbances and land-surface interactions. Recent advances in computational power, as well as data collection, storage, and distribution capabilities, have led to an improved ability to include these effects at a higher fidelity, and modern digital signal processing techniques have led to an improved ability to assess the utility of including them. This session seeks contributions covering advancements in measurement, modelling, and prediction techniques pertinent to the interaction of radio waves with the ionosphere in either a skywave or transionospheric propagation mode. Contributions highlighting improvements in our ability to include and understand the earth system’s interactions with these propagation modes are especially encouraged.
Primary Convener:  James C Jones, Northrop Grumman Corporation Bellevue, Bellevue, NE, United States
Conveners:  Jonah J Colman, Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States and Ethan S Miller, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Chairs:  James C Jones, Northrop Grumman Corporation Bellevue, Bellevue, NE, United States and Jonah J Colman, Air Force Research Laboratory Albuquerque, Albuquerque, NM, United States
OSPA Liaison:  Ethan S Miller, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Index Terms:

Abstracts Submitted to this Session:

David C Munton1, Roy S Calfas1, Thomas Gaussiran II2, David Rainwater3, Amy M Flesichmann3 and Jacob R Schofield3, (1)Univ Texas, Austin, TX, United States, (2)University of Texas at Austin, Austin, TX, United States, (3)U Texas/Applied Research Labs, Austin, TX, United States
Stephen Roland Kaeppler1, Russell B Cosgrove2, Cecile Mackay1, Roger H Varney3, Elizabeth A Kendall4 and Michael J Nicolls1, (1)SRI International Menlo Park, Menlo Park, CA, United States, (2)University of Central Florida and SRI International, Menlo Park, CA, United States, (3)University of California Los Angeles, Atmospheric and Oceanic Sciences, Los Angeles, CA, United States, (4)University of Central Florida, Orlando, CA, United States
David L Hysell, Cornell University, Earth and Atmospheric Sciences, Ithaca, NY, United States, Marco A Milla, University of Illinois at Urbana Champaign, Electrical and Computer Engineering, Urbana, United States and Juha Vierinen, The Arctic University of Norway, Department of Physics and Technology, Tromsø, Norway
Roland T Tsunoda, SRI International Palo Alto, Palo Alto, CA, United States
Yu-Ming Yang1, Meegyeong Paik1, Kamal Oudrhiri2, Dustin Buccino1 and Daniel S Kahan3, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Gareth William Perry1, Ethan S Miller2, Harry Gordon James3, Andrew David Howarth1, Jean-Pierre St-Maurice4 and Andrew W Yau1, (1)University of Calgary, Calgary, AB, Canada, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)Retired, Washington, DC, United States, (4)University of Saskatchewan, Saskatoon, SK, Canada
Raymond A Greenwald, Virginia Tech, Sykesville, MD, United States, Nathaniel A Frissell, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States and Sebastien de Larquier, Netflix, Los Gatos, CA, United States

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