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By Charles R. Chappell, Robert W. Schunk, Peter M. Banks, Richard M. Thorne, James L. Burch

Over a part century of exploration of the Earth’s house setting, it has turn into obvious that the interplay among the ionosphere and the magnetosphere performs a dominant function within the evolution and dynamics of magnetospheric plasmas and fields. curiously, it was once lately came upon that this similar interplay is of basic significance at different planets and moons through the sun method. in line with papers provided at an interdisciplinary AGU Chapman convention at Yosemite nationwide Park in February 2014, this quantity presents an highbrow and visible trip via our exploration and discovery of the paradigm-changing position that the ionosphere performs in picking the filling and dynamics of Earth and planetary environments. The 2014 Chapman convention marks the fortieth anniversary of the preliminary magnetosphere-ionosphere coupling convention at Yosemite in 1974, and hence offers a 4 decade viewpoint of the development of house technology examine in figuring out those basic coupling strategies. electronic video hyperlinks to a web archive containing either the 1974 and 2014 conferences are awarded all through this quantity to be used as an ancient source by means of the overseas heliophysics and planetary technology communities.

Topics coated during this quantity include:

  • Ionosphere as a resource of magnetospheric plasma
  • Effects of the low strength ionospheric plasma at the balance and production of the extra full of life plasmas
  • The unified worldwide modeling of the ionosphere and magnetosphere on the Earth and different planets
  • New wisdom of those coupled interactions for heliophysicists and planetary scientists, with a cross-disciplinary strategy concerning complex size and modeling techniques

Magnetosphere-Ionosphere Coupling within the sunlight System is a priceless source for researchers within the fields of house and planetary technological know-how, atmospheric technology, area physics, astronomy, and geophysics.

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Vaivads, et al. (1994), Transverse ion energization and wave emissions observed by the Freja satellite, Geophys. Res. Lett. 21, 1915–1918. A. M. Kintner, et al. (1992), Bursts of transverse ion acceleration at rocket altitudes, Geophys. Res. Lett. 19, 413–416. Banks, P. , and G. Kockarts (1973), Aeronomy, Part B, Academic Press, New York, NY, USA. Banks, P. , and T. E.  Geophys. 1029/JA073i021p06846. Bates, H. F. (1974), Atmospheric expansion from Joule heating, Planet. , 22, 925. , B. Klecker, W.

1979), Transversely accelerated ions: an ionospheric source of hot magnetospheric ions, J. Geophys. Res. 84, 4229–4237. , and M. Scherer (1971), Simple model for an ion‐ exosphere in an open magnetic field, Phys. Fluids, 14, 1683–1694. , W. K. Peterson, T. Chang, R. W. Schunk, A. R. Barakat, H. G. Demars, and G. V.  Atmos. Solar Terr. , 69, 1901–1935. Liu, H. , S. Y. Ma, K. Schlegel (2001), Diurnal, seasonal, and geomagnetic variations of large field‐aligned ion upflows in the high‐latitude ionospheric F‐region, J.

Published 2017 by John Wiley & Sons, Inc. 1 Schematic summary of satellite, rocket, and ground‐based radar observations of ion outflows in different altitude regions and different phases of Solar Cycle 20‐23. 7. by hydrodynamic [Banks and Holzer, 1968; Marubashi, 1970] and kinetic polar wind models [Lemaire and Scherer, 1971] in the 1960s. These early models laid the conceptual foundation for subsequent semi‐kinetic and transport‐ equations based models and recent three‐dimensional time‐dependent models [cf.

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