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Shadrian B. Strong, Ph.D. - Publications

Affiliations: 
2008 Astronomy University of Texas at Austin, Austin, Texas, U.S.A. 
Area:
Astronomy and Astrophysics, Fluid and Plasma
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6 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2014 Martin CA, Brown DM, Thomas ME, Strong S, Lohr MB. FTIR characterization of atmospheric fluctuations along slant paths Proceedings of Spie - the International Society For Optical Engineering. 9071. DOI: 10.1117/12.2050644  0.326
2014 Strong SB, Brown AM. Developing a broad spectrum atmospheric aerosol characterization for remote sensing platforms over desert regions Proceedings of Spie - the International Society For Optical Engineering. 9071. DOI: 10.1117/12.2050575  0.391
2012 Kelly MA, Osei-Wusu K, Spisz TS, Strong S, Setters N, Gibson DM. Assimilation of nontraditional datasets to improve atmospheric compensation Proceedings of Spie - the International Society For Optical Engineering. 8380. DOI: 10.1117/12.919366  0.393
2009 Harper GM, Richter MJ, Ryde N, Brown A, Brown J, Greathouse TK, Strong S. Texes observations of m supergiants: Dynamics and thermodynamics of wind acceleration Astrophysical Journal. 701: 1464-1483. DOI: 10.1088/0004-637X/701/2/1464  0.455
2007 Massey P, Mcneill RT, Olsen KAG, Hodge PW, Blaha C, Jacoby GH, Smith RC, Strong SB. A survey of local group galaxies currently forming stars. III. A search for luminous blue variables and other Hα emission-line stars Astronomical Journal. 134: 2474-2503. DOI: 10.1086/523658  0.366
2006 Richter MJ, Lacy JH, Jaffe DT, Mar DJ, Goertz J, Möller WM, Strong S, Greathouse TK. Development and future use of the echelon-cross-echelle spectrograph on SOFIA Proceedings of Spie - the International Society For Optical Engineering. 6269. DOI: 10.1117/12.670559  0.38
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