By J. D. Huba, R. W. Schunk, G. V. Khazanov
Published through the yankee Geophysical Union as a part of the Geophysical Monograph sequence, quantity 201.
Modeling the Ionosphere-Thermosphere System brings jointly for the 1st time an in depth description of the physics of the IT approach along side numerical ideas to resolve the advanced approach of equations that describe the approach, in addition to problems with present curiosity. quantity highlights contain discussions of:
- Physics of the ionosphere and thermosphere IT method, and the numerical tips on how to remedy the elemental equations of the IT system
- The physics and numerical ways to ensure the worldwide electrodynamics of the IT system
- The reaction of the IT process to forcings from under (i.e., the reduce surroundings) and from above (i.e., the magnetosphere)
- The physics and numerical easy methods to version ionospheric irregularities
- Data assimilation options, comparability of version effects to info, weather variability reports, and purposes to area weather
Providing a transparent description of the physics of the program in numerous tutorial-like articles, Modeling the Ionosphere-Thermosphere System is of price to the higher surroundings technological know-how group in most cases. Chapters describing info of the numerical equipment used to unravel the equations that describe the IT method make the amount priceless to either energetic researchers within the box and students.
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Released by means of the yank Geophysical Union as a part of the Geophysical Monograph sequence, quantity 201. Modeling the Ionosphere-Thermosphere method brings jointly for the 1st time an in depth description of the physics of the IT method along side numerical ideas to resolve the advanced approach of equations that describe the method, in addition to problems with present curiosity.
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Additional resources for Modeling the Ionosphere-Thermosphere
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Electron recombination is particularly important because the molecular ion loss rates are proportional to the electron density, and the peak electron density increases by almost an order of magnitude from solar minimum to solar maximum. In the F1 region of the ionosphere between 120 and 200 km, solar cycle increases in ion production rate due to increasing solar EUV intensity are largely offset by increased attenuation from the increased O and N2 column densities. The solar cycle variation of the molecular ion densities is largest in the region due to the large solar cycle increases in the soft X-ray irradiances that create a large increase in photoelectron ﬂux.
Scott, G. B. , D. A. Fairley, D. B. Milligan, C. G. Freeman, and M. J. McEwan (1999), Gas phase reactions of some positive ions with atomic and molecular oxygen and nitric oxide at 300 K, J. Phys. Chem. A, 103, 7470–7473. Solomon, S. C. (2006), Numerical models of the E-region ionosphere, Advances in Space Research, 37, 1031–1037, doi:10. 040. Solomon, S. , and L. Qian (2005), Solar extreme-ultraviolet irradiance for general circulation models, J. Geophys. 1029/2005JA011160. , and D. G. Torr (1978), Nonthermal rate coefﬁcients in the ionosphere: The reactions of O+ with N2, O2, and NO, J.
Modeling the Ionosphere-Thermosphere by J. D. Huba, R. W. Schunk, G. V. Khazanov