On the Need to Reparametrize the OVATION Prime (2010) Auroral Precipitation Model-Reference-Cited by-同舟云学术

On the Need to Reparametrize the OVATION Prime (2010) Auroral Precipitation Model

Published:2021-03 Issue:3 Volume:46 Page:194-199
ISSN:1068-3739
Container-title:Russian Meteorology and Hydrology
language:en
Short-container-title:Russ. Meteorol. Hydrol.

Author:

Nikolaev A. V.

Publisher

Allerton Press

Subject

Atmospheric Science,Fluid Flow and Transfer Processes,Water Science and Technology

Link

https://link.springer.com/content/pdf/10.3103/S1068373921030080.pdf

Reference35 articles.

1. D. H. Brautigam, M. S. Gussenhoven, and D. A. Hardy, “A Statistical Study on the Effects of IMF Bz and Solar Wind Speed on Auroral Precipitation,” J. Geophys. Res., 96 (1991).

2. J. F. Carbary, T. Sotirelis, P. T. Newell, and C.-I. Meng, “Auroral Boundary Correlations between UVI and DMSP,” J. Geophys. Res., 108 (2003).

3. S. W. H. Cowley, “Magnetosphere–Ionosphere Interactions: A Tutorial Review,” in Magnetospheric Current Systems, Ed. by S.-I. Ohtani, R. Fujii, M. Hesse, and R. L. Lysak (2013).

4. T. N. Davis and M. Sugiura, “Auroral Electrojet Activity Index AE and Its Universal Time Variations,” J. Geophys. Res., 71 (1966).

5. D. S. Evans, “Global Statistical Patterns of Auroral Phenomena,” inQuantitative Modeling of Magnetospheric-Ionospheric Coupling Processes, Ed. by Y. Kamide and R. A. Wolf (Kyoto Sangyo Univ., Kyoto, Japan, 1987).

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