SA51A:
Understanding Traveling Ionospheric Disturbances (TIDs) I


Submit an Abstract to this Session


Session ID#: 61556

Session Description:
Traveling ionospheric disturbances (TIDs) are an important part of the upper  atmospheric variability.  They occur on a regular basis across high, mid-, and equatorial latitudes. They are believed to be a manifestation of atmospheric waves such as AGWs and most of the known TID properties are well within the expected regime of AGWs. Excitation sources of TIDs/AGWs are numerous, but may be classified as from “above” and “below.” This session will provide a forum for reporting recent progress on TID studies and envisioning future research directions. We solicit contributions on various TID topics including: LSTIDs and storm-time traveling atmosphere disturbances (TADs), MSTIDs and E-F region electrodynamic coupling at mid- and low latitudes, man-made space weather induced TIDs, TIDs associated with the solar terminator, solar eclipse, and solar flares. Reports of ground-based and in-situ observations as well as simulations of ionosphere-thermosphere disturbances associated with TIDs are all welcome.
Primary Convener:  Shunrong Zhang, MIT Haystack Observatory, Westford, MA, United States
Convener:  Anthea Coster, MIT Haystack Observatory, Westford, MA, United States
Primary Liaison:  Shunrong Zhang, MIT Haystack Observatory, Westford, MA, United States
Chairs:  Shunrong Zhang, MIT Haystack Observatory, Westford, MA, United States and Anthea Coster, MIT Haystack Observatory, Westford, MA, United States
OSPA Liaison:  Shunrong Zhang, MIT Haystack Observatory, Westford, MA, United States

Abstracts Submitted to this Session:

Joseph Helmboldt, US Naval Research Laboratory, Washington, DC, United States, Tracy Clarke, Naval Research Lab DC, 7200, Washington, DC, United States, Wendy Peters, US Naval Research Laboratory, Code 7213, Washington, DC, United States, Walter Brisken, Long Baseline Observatory, Socorro, United States and VLA Low-band Ionosphere and Transient Experiment (VLITE) team
Yasunobu Miyoshi, Kyushu University, Fukuoka, Japan, Hidekatsu Jin, NICT National Institute of Information and Communications Technology, Tokyo, Japan, Hitoshi Fujiwara, Seikei University, Tokyo, Japan and Hiroyuki Shinagawa, Kyushu University, International Research Center for Space and Planetary Environmental Science, Fukuoka, Japan
Jonathan B Snively1, Christopher James Heale1 and Matthew D Zettergren2, (1)Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, (2)Embry-Riddle Aeronautical University, Department of Physical Sciences, Daytona Beach, FL, United States
Feng Ding, Institute of Geology and Geophysics Chinese Academy of Sciences, Beijing, China and Haitao Liu, Macau University of Science and Technology, Macau, China
Yuichi Otsuka1, Dr. Atsuki Shinbori2, Takuya Tsugawa3 and Michi Nishioka3, (1)ISEE, Nagoya University, Nagoya, Japan, (2)Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan, (3)NICT National Institute of Information and Communications Technology, Tokyo, Japan
Viswanathan Lakshmi Narayanan1, Shiokawa Kazuo2, Yuichi Otsuka2 and Dave Neudegg3, (1)National Atmospheric Research Laboratory, Gadanki, India, (2)ISEE, Nagoya University, Nagoya, Japan, (3)University of Adelaide, Adelaide, Australia
Larry R Lyons1, Yukitoshi Nishimura2, Shunrong Zhang3, Anthea Coster3, Asti Bhatt4, Elizabeth A Kendall5 and Yue Deng6, (1)University of California Los Angeles, Department of Atmospheric and Oceanic Sciences, Los Angeles, CA, United States, (2)Boston University, Boston, United States, (3)MIT Haystack Observatory, Westford, MA, United States, (4)SRI International, Menlo Park, United States, (5)SRI International, Menlo Park, CA, United States, (6)University of Texas Arlington, Arlington, United States
Elizabeth A Kendall, University of Central Florida, Orlando, CA, United States and Asti Bhatt, SRI International, Menlo Park, United States

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