Диссертация (1097736), страница 41
Текст из файла (страница 41)
- Ì: Ìèð, 1979.416 ñ.[169] Ñïðàâî÷íèê ïî ëàçåðàì. / Ïîä ðåä. À. Ì. Ïðîõîðîâà. Ì.: Ñîâ. Ðàäèî, 1978. 504 ñ.[170] Áèñÿðèí Â. Ï., Ñîêîëîâ À. Â., Ñóõîíèí Å. Â. è äð. Îñëàáëåíèå ëàçåðíîãîèçëó÷åíèÿ â ãèäðîìåòåîðàõ. Ì.: Íàóêà, 1977.281[171] Èâàíîâ À. Ï. Îïòèêà ðàññåèâàþùèõ ñðåä. Ìèíñê: Íàóêà è òåõíèêà, 1969.592 ñ.[172] Áàðòåíåâà Î. Ä.
Èíäèêàòðèñû ðàññåÿíèÿ ñâåòà â ïðèçìåííîì ñëîå àòìîñôåðû // Èçâ. ÀÍ ÑÑÑÐ. Ñåð. ãåîôèç. 1960. Ñ. 1852-1865.[173] Gordon G., Richard W. Integrating nephelometer and implication // Appl.Opt. 1985. V. 24. P.2721-2730.[174] Îøëàêîâ Â. Ã., Îøëàêîâ Â. Ê., Åðåìèíà Ò. À. Îïòèìàëüíûå ïîëÿðèçàöèîííûå õàðàêòåðèñòèêè ïðèáîðîâ, ðåãèñòðèðóþùèõ ðàññåÿííîå èçëó÷åíèå// Îïòèêà àòìîñôåðû è îêåàíà. 2007. Ò. 20. C.635640[175] Îøëàêîâ Â. Ã., Öâûê Ð. Ø., Èëþøèí ß. À. Îïòè÷åñêàÿ èíñòðóìåíòàëüíàÿñïèñòåìà îðèåíòèðîâàíèÿ â óñëîâèÿõ íåäîñòàòî÷íîé âèäèìîñòè.
// Ñáîðíèê òðóäîâ íàó÷íî-òåõíè÷åñêîé êîíôåðåíöèè "Òåõíè÷åñêîå çðåíèå â ñèñòåìàõ óïðàâëåíèÿ 2012"Ìîñêâà, ÈÊÈ ÐÀÍ. C.16-25.[176] Henyey L. G., Greenstein J. L. Diuse radiation in the galaxy. // Astrophys.J. 1941. V.93. P.7083.[177] Áðàâî-Æèâîòîâñêèé Ä. Ì., Äîëèí Ë. Ñ., Ëó÷èíèí À. Ã., Ñàâåëüåâ Â. À.Î ñòðóêòóðå óçêîãî ïó÷êà ñâåòà â ìîðñêîé âîäå. // Èçâ. ÀÍ ÑÑÑÐ Ôèçèêààòìîñôåðû è îêåàíà. 1969. Ò.5. C.160-167.[178] Ëåáåäåâ Â. È. Î êâàäðàòóðàõ íà ñôåðå.
// Æóðíàë âû÷èñëèòåëüíîé ìàòåìàòèêè è ìàòåìàòè÷åñêîé ôèçèêè. 1976. Ò.16. Ñ.293.[179] Mishchenko M. I. Polarization eects in weak localization of light: Calculationof the copolarized and depolarized backscattering enhancement factors. //Phys. Rev. B. 1991. V.44. P.1259712600.[180] Mishchenko M. I. Enhanced backscattering of polarized light from discreterandom media: calculations in exactly the backscattering direction. // J. Opt.Soc. Am.
A. 1992. V.9. P.978982.[181] Áåêåôè Äæ. Ðàäèàöèîííûå ïðîöåññû â ïëàçìå. M.:Ìèð, 1971. 438 c.282[182] Smerd S. F., Westfold K. C. The characteristics of radio-frequency radiationin an ionized gas, with applications to the transfer of radiation in the solaratmosphere. // Phil. Mag. 1949. V.40. P.831848.[183] Ferwerda H. A. The radiative transfer equation for scattering media with aspatially varying refractive index.
// Journal of Optics A: Pure and AppliedOptics. 1999. V.1. P.L1.[184] Tualle J. M., Tinet E. Derivation of the radiative transfer equation forscattering media with a spatially varying refractive index. //OpticsCommunications. 2003. V.228. P.3338.[185] Shendeleva M. L. Radiative transfer in a turbid medium with a varyingrefractive index: comment. // J. Opt. Soc. Am.
A. 2004. V.21. P.24642467.[186] Liu L., Zhang L., Tan H. Radiative transfer equation for graded index mediumin cylindrical and spherical coordinate systems. // Journal of QuantitativeSpectroscopy and Radiative Transfer. 2006. V.97. P.446456.[187] Liu L., Zhang H., Tan H. Monte-Carlo discrete curved ray-tracing method forradiative transfer in an absorbing-emitting semitransparent slab with variablespatial refractive index. // Journal of Quantitative Spectroscopy and RadiativeTransfer. 2004.
V.84. P.357362.[188] Zhu K.-Y., Huang Y., Wang J. Curved ray tracing method for one-dimensionalradiative transfer in the linear-anisotropic scattering medium with gradedindex. // Journal of Quantitative Spectroscopy and Radiative Transfer. 2011.V.112., P.377383.[189] Sassaroli A., Martelli F. Equivalence of four Monte-Carlo methods for photonmigration in turbid media.
// J. Opt. Soc. Am. A. 2012. V.29. P.21102117.[190] Haskell R. C., Svaasand L. O., Tsay T.-T., Feng T.-C., McAdams M. S.,Tromberg B. J. Boundary conditions for the diusion equation in radiativetransfer. // J. Opt. Soc. Am. A. V.11. P.27272741. 1994.[191] Ýëüñãîëüö Ë. Ý. Äèôôåðåíöèàëüíûå óðàâíåíèÿ è âàðèàöèîííîå èñ÷èñëåíèå. Ì.: Íàóêà, 1969. 424 ñ.283[192] Kim A. D., Moscoso M.
Backscattering of beams by forward-peaked scatteringmedia. // Opt. Lett. 2004. V.29. P.7476.[193] Campbell S. D., O'Connell A. K., Rutherford G. H., Grobe R. Impact of largeangle scattering on diusively backscattered halos. // Opt. Lett. 2007.
V.32.P.560562.[194] Wiersma D. S., van Albada M. P., van Tiggelen B. A., Lagendijk A.,Experimental evidence for recurrent multiple scattering events of light indisordered media. // Phys. Rev. Lett. 1995. V.74. P.41934196.[195] Áîðåí Ê., Õàôìåí Ä. Ïîãëîùåíèå è ðàññåÿíèå ñâåòà ìàëûìè ÷àñòèöàìè.Ì.: Ìèð, 1986. 664 c.[196] Berkovits R., Kaveh M.
Weak localisation of photons in a disordered twodimensional medium. // J. Phys. C. 1987. V.20. P.L181L185.[197] Freund I. , Rosenbluh M., Berkovits R., Kaveh M. Coherent backscatteringof light in a quasi-two-dimensional system. // Phys. Rev. Lett. 1988. V.61.P.12141217.[198] Gorodnichev E. E., Dudarev S. L., Rogozkin D. B. Coherent backscatteringenhancement under conditions of weak wave localisation in disordered 3D and2D systems.
// Sov. Phys. JETP 1989. V.69. P.481490.[199] Mishchenko M. I. Polarized light transfer in a medium containing perfectlyoriented elongated particles. // Kinem. Phys. Celest. Bodies. 1987. V.3.P.5362.[200] Mishchenko M. I., Yanovitskij E. G. Polarized light transfer in a mediumcontaining perfectly oriented elongated particles. General theory. 'Rayleigh'scattering. // Kinem. Phys. Celest. Bodies. V.4.
P.1929. 1988.[201] Mishchenko M. I., Dlugach J. M., Yanovitskij E. G. Multiple light scattering bypolydispersions of randomly distributed perfectly-aligned, innite Mie cylindersilluminated perpendicularly to their axes // J. Quantum Spectrosc. Radiat.Transfer. V.47. P.401410. 1992.284[202] Alexandrov M. D., Remizovich V. S., Rogozkin D. B. Multiple light scatteringin a two-dimensional medium with large scatterers. // J. Opt. Soc.
Am. A.1993. V.10. P.2602-2610.[203] van Wijk K., Haney M. M., Scales J. A. 1D energy transport in a stronglyscattering laboratory model. // Physical Review E. 2004. V.69. P.036611.[204] Áóäàê Â.Ï., Èëþøèí ß.À. Óñòðàíåíèå îñîáåííîñòåé ðåøåíèÿ òðåõìåðíûõêðàåâûõ çàäà÷ òåîðèè ïåðåíîñà èçëó÷åíèÿ. // Òåïëîâûå ïðîöåññû â òåõíèêå. 2010. Ò.
2. Ñ. 471-474.[205] Abshire J. B., Sun X., Afzal R. S. Mars Orbiter Laser Altimeter: ReceiverModel and Performance Analysis. // Appl. Opt. 2000. V.39. P.2449-2460.[206] Kreslavsky M. A., Head, J. W.. Kilometer-scale roughness of Mars: resultsfrom MOLA data analysis. // J. Geophys. Res. 2000. V.105.
P.26,69526,711.[207] Davies D. W. The Mars water cycle. // Icarus. 1981. V.45. P.398414.[208] Farmer C. B., Davies D. W., LaPorte D. D. Mars: Northern summer ice cap water vapor observations from Viking 2. // Science. 1976. V.194. P.13391340.[209] Kieer H.H., Chase S. C., Martin T. Z., Miner E. D., Palluconi F. D. Martiannorth pole summer temperatures: Dirty water ice. // Science. 1976.
V.194.P.13411343.[210] Paige D. A., Barchman J. E., Keegan K. D.. Thermal and albedo mapping ofthe polar regions of Mars using Viking thermal mapper observations. 1. Northpolar region. // J. Geophys. Res. 1994. V.99. P.25,95925,991.[211] Paige D. A., Keegan K. D.. Thermal and albedo mapping of the polar regionsof Mars using Viking Thermal Mapper observations.
2. South polar region. //J. Geophys. Res. 1994. V.99. P.25,99326,013.[212] Kieer, H. H. H2 O grain size and the amount of dust in Mars' residual northpolar cap. // J. Geophys. Res. 1990. V.95. P.14811493.[213] Malin M. C. Density of martian north polar layered deposits: implications forcomposition. // Geophys. Res. Lett. 1986. V.13. P.444447.285[214] Schenk P. M. Moore J. M. Stereo topography of the south polar region of Mars:volatile inventory and Mars Polar Lander landing site. // J. Geophys.
Res.V.105. P.24,52924,546. 2000.[215] Muhleman D. O., et al. Radar investigation of Mars, Mercury and Titan. //Ann. Rev. Earth Planet Sci. 1995. V.23. P. 337374.[216] Cliord S. M., et al. The state and future of Mars polar science andexploration. // Icarus. 2000. V.144. P.210242.[217] Milkovich, S.
M., Head J .W. North Polar Cap of Mars: Polar LayeredDeposit Characterization and Identication of a Fundamental Climate Signal.// J. Geophys. Res. 2005. V.110. P.1005.[218] Blasius K. R., Cutts J. A., Howard A. D. Topography and stratigraphy ofmartian polar deposits. // Icarus. 1982. V.50. P.140160.[219] Skorov Yu. V. et al. Stability of water ice under a porous nonvolatile layer:implications to the south polar layered deposits of Mars. // Planetary andSpace Science. 2001. V.49. P.5963.[220] Thomas P. C. et al.
North-south geological dierences between the residualpolar caps on Mars. // Nature. 2000. V.404. P.161164.[221] Cutts J.A., Lewis B. H. Models of climate cycles recorded in martian polarlayered deposits. // Icarus. 1982. V.50. P.216244.[222] Greve R. Waxing and Waning of the Perennial North Polar H2 O Ice Cap ofMars over Obliquity Cycles. // Icarus. 2000. V.131. P.419431.[223] Fishbaugh K. E. Hvidberg C. S. Martian north polar layered depositsstratigraphy: Implications for accumulation rates and ow. J. Geophys.
Res.2006. V.111. P.E06012.[224] Johnson C. L., Solomon S. C., Head J. W., Phillips R. J., Smith D. E., ZuberM. T. Lithospheric loading by the northern polar cap of Mars. // Icarus. 2000.V.144. P.313328.286[225] Campbell, B. A., Ghent R. R., Shepard M. K. Limits of inference of Marssmall scale topography from MOLA data. // Geophysical Research Letters.2003. V.30. P.1115.[226] Èëþøèí ß. À.
![](https://s.studizba.com/z.php?f=/templates/si/i/noavatar.png&w=100&h=100&t=1"){kind=avatar}
