fresnel reflection by wavy water

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Proceedings of the International Geoscience and Remote Sensing Symposium IGARSS 2000, 24-28 July 2000, Honolulu, Hawaii, USA, ed. Tammy I. Stein, IEEE Cat. No. 00CH37120, ISBN 0-7803-6359-0, IEEE, Piscataway, NJ, USA, 2000. 0-7803-6359-0/00/$10.00 © 2000 IEEEE 1863 Fresnel reflection by wavy sea surface Vladimir I. Haltrin, Walton E. McBride III,° and Alan D. Weidemann, Naval Research Laboratory, Ocean Sciences Branch, Code 7333 Stennis Space Center, MS 39529-5004, USA. e-mail: <[email protected]> ° Planning Systems Inc., 115 Christian Lane, Slidell, LA 70458, USA Abstract In studying light and image transfer in sea waters, the influence of Fresnel surface reflection is as significant as scattering and absorption phenomena. In these cases knowledge of the reflective properties of sea surface at different wind speeds is very important. At present, little is published about these properties. We present here results of numerical modeling of angular reflection coefficients of sea water as a function of zenith angle of illumination and wind speed. INTRODUCTION The ray-tracing computer model was developed and implemented as slopes and elevations. The model used the Pierson-Moskowitz (PM) [1] and Paul Hwang (PH) [2] wave height spectrums in order to generate a realistic sea surface {see Fig. 1 and Eqs. (1) and (2)}. The Fresnel reflection coefficients were averaged over 10000 pixels of sea surface areas and 80 time realizations to produce resulting angular distributions of Fresnel reflection coefficient. The Pierson-Moskowitz [1] wave energy spectrum is Figure 1. Comparison of Pierson-Moskowitz and Paul Hwang spectrums at windspeed of 4 m/s. defined as: χ PM k k g uk () . exp . = 0 00405 0 74 3 2 4 2 (1) here g m s = 98 . / is a gravitational acceleration, u is a windspeed in m s / , k g u = / is a wavenumber in m 1 . The Paul Hwang [2] wave energy spectrum is defined as: χ PH k k k gu u k gu k uk k u g k k uk k () . , , . , ., . , . ., () . . , , . , . = < < < + ( ) < 1 10 5 45 1 74 16 0 6 96 16 0 100 0 2 0 682 0 00007 100 900 7 48 10 900 4 2 2 2 2 6 3 This spectrum is specifically tailored to produce correct values of mean square slopes of ocean waves. Figure 2. Comparison of Fresnel reflection coefficients of wavy surface calculated with energy spectrums and Cox and Munk distribution of slopes.

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Fresnel Reflection

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  • Proceedings of the International Geoscience and Remote Sensing Symposium IGARSS 2000, 24-28 July 2000, Honolulu,Hawaii, USA, ed. Tammy I. Stein, IEEE Cat. No. 00CH37120, ISBN 0-7803-6359-0, IEEE, Piscataway, NJ, USA, 2000.

    0-7803-6359-0/00/$10.00 2000 IEEEE1863

    Fresnel reflection by wavy sea surface

    Vladimir I. Haltrin, Walton E. McBride III, and Alan D. Weidemann,

    Naval Research Laboratory, Ocean Sciences Branch, Code 7333Stennis Space Center, MS 39529-5004, USA. e-mail:

    Planning Systems Inc., 115 Christian Lane, Slidell, LA 70458, USAAbstract In studying light and image transfer in seawaters, the influence of Fresnel surface reflection is assignificant as scattering and absorption phenomena. In thesecases knowledge of the reflective properties of sea surface atdifferent wind speeds is very important. At present, little ispublished about these properties. We present here results ofnumerical modeling of angular reflection coefficients of seawater as a function of zenith angle of illumination and windspeed.

    INTRODUCTION

    The ray-tracing computer model was developed andimplemented as slopes and elevations. The model used thePierson-Moskowitz (PM) [1] and Paul Hwang (PH) [2] waveheight spectrums in order to generate a realistic sea surface{see Fig. 1 and Eqs. (1) and (2)}. The Fresnel reflectioncoefficients were averaged over 10000 pixels of sea surfaceareas and 80 time realizations to produce resulting angulardistributions of Fresnel reflection coefficient.

    The Pierson-Moskowitz [1] wave energy spectrum is

    Figure 1. Comparison of Pierson-Moskowitz and PaulHwang spectrums at windspeed of 4 m/s.

    defined as:

    PM k kg

    u k( )

    .exp

    .=

    0 00405 0 743

    2

    4 2 (1)

    here g m s= 9 8. / is a gravitational acceleration, u is awindspeed in m s/ , k g u= / is a wavenumber in m1 .

    The Paul Hwang [2] wave energy spectrum is defined as:

    PH k k

    k g u

    u k g u k

    u k k

    u g k k

    u k k

    ( )

    . , ,

    . , . ,

    . , . . , ( )

    . . , ,

    . , .

    =