TY - JOUR
T1 - The geospace response to variable inputs from the lower atmosphere
T2 - a review of the progress made by Task Group 4 of CAWSES-II
AU - Oberheide, Jens
AU - Shiokawa, Kazuo
AU - Gurubaran, Subramanian
AU - Ward, William E.
AU - Fujiwara, Hitoshi
AU - Kosch, Michael J.
AU - Makela, Jonathan J.
AU - Takahashi, Hisao
N1 - Funding Information:
JO, KS, and SG are grateful for the enthusiasm and contributions of all 250 members of TG4, especially the project leaders W. Ward, M. A. Abdu, J. Chau, J. Makela, H. Takahashi, D. Pancheva, M. Yamamoto, H. Fujiwara, and M. Kosch. Our special acknowledgement goes to Dr. Michi Nishioka who edited the quarterly newsletter. JM and HT thank all of the LONET and SpreadFEx-2 campaign participants. JM and HT acknowledge the COSMIC data center team who provided the TEC data. The Pameungpeuk MF radar data were provided through IUGONET under agreement of RISH, Kyoto University. JO was supported by NSF award 1139048 and NASA grants NNX11AJ13G and NNH12CF66C. KS is supported by the JSPS Grants-in-Aid for Scientific Research (20244080, 23403009, and 25247080), JSPS Core-to-Core Program, B. Asia-Africa Science Platforms, and the STEL Cooperative and IUGONET Projects from MEXT, Japan.
Publisher Copyright:
© 2015, Oberheide et al.; licensee Springer.
PY - 2015/12/1
Y1 - 2015/12/1
N2 - The advent of new satellite missions, ground-based instrumentation networks, and the development of whole atmosphere models over the past decade resulted in a paradigm shift in understanding the variability of geospace, that is, the region of the atmosphere between the stratosphere and several thousand kilometers above ground where atmosphere-ionosphere-magnetosphere interactions occur. It has now been realized that conditions in geospace are linked strongly to terrestrial weather and climate below, contradicting previous textbook knowledge that the space weather of Earth's near space environment is driven by energy injections at high latitudes connected with magnetosphere-ionosphere coupling and solar radiation variation at extreme ultraviolet wavelengths alone. The primary mechanism through which energy and momentum are transferred from the lower atmosphere is through the generation, propagation, and dissipation of atmospheric waves over a wide range of spatial and temporal scales including electrodynamic coupling through dynamo processes and plasma bubble seeding. The main task of Task Group 4 of SCOSTEP's CAWSES-II program, 2009 to 2013, was to study the geospace response to waves generated by meteorological events, their interaction with the mean flow, and their impact on the ionosphere and their relation to competing thermospheric disturbances generated by energy inputs from above, such as auroral processes at high latitudes. This paper reviews the progress made during the CAWSES-II time period, emphasizing the role of gravity waves, planetary waves and tides, and their ionospheric impacts. Specific campaign contributions from Task Group 4 are highlighted, and future research directions are discussed.
AB - The advent of new satellite missions, ground-based instrumentation networks, and the development of whole atmosphere models over the past decade resulted in a paradigm shift in understanding the variability of geospace, that is, the region of the atmosphere between the stratosphere and several thousand kilometers above ground where atmosphere-ionosphere-magnetosphere interactions occur. It has now been realized that conditions in geospace are linked strongly to terrestrial weather and climate below, contradicting previous textbook knowledge that the space weather of Earth's near space environment is driven by energy injections at high latitudes connected with magnetosphere-ionosphere coupling and solar radiation variation at extreme ultraviolet wavelengths alone. The primary mechanism through which energy and momentum are transferred from the lower atmosphere is through the generation, propagation, and dissipation of atmospheric waves over a wide range of spatial and temporal scales including electrodynamic coupling through dynamo processes and plasma bubble seeding. The main task of Task Group 4 of SCOSTEP's CAWSES-II program, 2009 to 2013, was to study the geospace response to waves generated by meteorological events, their interaction with the mean flow, and their impact on the ionosphere and their relation to competing thermospheric disturbances generated by energy inputs from above, such as auroral processes at high latitudes. This paper reviews the progress made during the CAWSES-II time period, emphasizing the role of gravity waves, planetary waves and tides, and their ionospheric impacts. Specific campaign contributions from Task Group 4 are highlighted, and future research directions are discussed.
KW - Geospace
KW - Gravity waves
KW - Ionosphere
KW - Planetary waves
KW - Thermosphere
KW - Tides
KW - Traveling atmospheric disturbances
KW - Traveling ionospheric disturbances
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U2 - 10.1186/s40645-014-0031-4
DO - 10.1186/s40645-014-0031-4
M3 - Review article
AN - SCOPUS:84943448789
SN - 2197-4284
VL - 2
JO - Progress in Earth and Planetary Science
JF - Progress in Earth and Planetary Science
IS - 1
M1 - 2
ER -