Found 120 results
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J. S. Evans, Strickland, D. J., and Huffman, R. E., Satellite remote sensing of thermospheric O/N 2 and Solar EUV: 2. Data analysis, Journal of Geophysical Research, vol. 100, no. A7, p. 12227, 1995.
R. W. Eastes, Emissions from the N2 Lyman-Birge-Hopfield bands in the earth's atmosphere, Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science, vol. 25, no. 5-6, pp. 523 - 527, 2000.
N. Curtis, Crowley, G., Christensen, A. B., Paxton, L. J., Robichaud, J., Barry, M. A., and Bust, G. S., Global Ultra-Violet Ionosphere-Thermosphere Observatory (GUVITO), in AGU Fall Meeting Abstracts, 2009.
D. J. Crain, Future data requirements of operational space weather systems, in Optical Science and Technology, the SPIE 49th Annual MeetingAtmospheric and Environmental Remote Sensing Data Processing and Utilization: an End-to-End System Perspective, Denver, CO, 2004.
R. J. Cox, Strickland, D. J., Evans, J. S., Wright, K. C., and Paxton, L. J., Continued development of radiance models and imaging software for the reduction, analysis, and visualization of space-based UV imaging data, in SPIE's 1994 International Symposium on Optics, Imaging, and InstrumentationUltraviolet Technology V, San Diego, CA, 1994.
J. Correira, Evans, J. S., and Strickland, D. J., {Comparison of solar energy flux Q$_{EUV}$ (łt} 45 nm) from SSUSI, GUVI, EVE, SEE, and SEM}, AGU Fall Meeting Abstracts, p. A927, 2011.
J. Correira, Strickland, D. J., Evans, J. S., Knight, H. K., and Hecht, J. H., A downward revision of a recently reported proton auroral LBH emission efficiency, Journal of Geophysical Research, vol. 116, no. A7, 2011.
J. Comberiate, Miller, E. S., Paxton, L. J., Makela, J. J., and Kelley, M. C., Coordinated Ground-and Space-based 3-D Electron Density Reconstruction and Plasma Bubble Imaging, in AGU Fall Meeting Abstracts, 2009.
J. Comberiate, Kelly, M. A., Miller, E., and Paxton, L., The Mesoscale Ionospheric Simulation Testbed (MIST) Regional Data Assimilation Model, in AGU Fall Meeting Abstracts, 2013.