By Gorden Videen, Yaroslav Yatskiv, Michael Mishchenko
ISBN-10: 1402023669
ISBN-13: 9781402023668
ISBN-10: 1402023685
ISBN-13: 9781402023682
Photopolarimetric distant sensing is essential in fields as varied as scientific diagnostics, astrophysics, atmospheric technology, environmental tracking and armed forces intelligence. The components thought of the following comprise: radiative move; dynamic structures; backscatter polarization; organic platforms; astrophysical phenomena; comets; and instrumentation. Subtopics comprise observational details together with deciding on morphology and chemistry, light-scattering types, and characterization methodologies. whereas this introductory textual content highlights the most recent advances during this multi-disciplinary subject, it's also a reference consultant for the complicated researcher.
Read Online or Download Photopolarimetry in Remote Sensing: Proceedings of the NATO Advanced Study Institute, held in Yalta, Ukraine, 20 September - 4 October 2003 (NATO Science Series II: Mathematics, Physics and Chemistry) PDF
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Extra info for Photopolarimetry in Remote Sensing: Proceedings of the NATO Advanced Study Institute, held in Yalta, Ukraine, 20 September - 4 October 2003 (NATO Science Series II: Mathematics, Physics and Chemistry)
Sample text
H. Poincaré (1892). Théorie Mathématique de la Lumière, Vol. 2 (Georges Carré, Paris). 44 M. I. MISHCHENKO AND L. D. TRAVIS 22. E. Whittaker (1987). A History of the Theories of Aether and Electricity, Vols. I and II (American Institute of Physics, New York). 23. D. Pye (2001). Polarised Light in Science and Nature (Institute of Physics Publishing, Bristol, UK). Evgeniy Zubko, Mark Thoreson, Vsevolod Ivanov, Pavel Litvinov, Oleg Dubovik, Valery Loiko, Matthew Easley, Olga Kalashnikova, Rosario Vilaplana, Ben Veihelmann, James McDonald, Hal Maring, Karine Chamaillard, Michael Mishchenko, and Tracy Smith (from left to right).
I. MISHCHENKO AND L. D. 6) where ∆ = ∆θ − ∆ϕ . 7) Substituting Eqs. 2) into Eq. 8) δ θ = ∆θ + knˆ ⋅ r, δ ϕ = ∆ϕ + knˆ ⋅ r. 9) where At any fixed point O in space, the endpoint of the real electric vector given by Eqs. 11) describes an ellipse with specific major and minor axes and orientation (see the top panel of Fig. 1). The major axis of the ellipse makes an angle ζ with the positive direction of the ϕ -axis such that ζ ∈ [0, π ). By definition, this orientation angle is obtained by rotating the ϕ -axis in the clockwise direction when looking in the direction of propagation, until it is directed along the major axis of the ellipse.
2: The polarizer transmission axes are rotated through an angle η ≥ 0 around nˆ in the clockwise direction when looking in the direction of propagation. 1. 2. 3. “rotate” the initial Stokes vector through the angle η in the clockwise direction in order to obtain the Stokes parameters of the original beam with respect to the polarizer axes; multiply the “rotated” Stokes vector by the original (non-rotated) polarizer Mueller matrix; and finally “rotate” the Stokes vector thus obtained through the angle −η in order to calculate the Stokes parameters of the resulting beam with respect to the laboratory coordinate system.
Photopolarimetry in Remote Sensing: Proceedings of the NATO Advanced Study Institute, held in Yalta, Ukraine, 20 September - 4 October 2003 (NATO Science Series II: Mathematics, Physics and Chemistry) by Gorden Videen, Yaroslav Yatskiv, Michael Mishchenko
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