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Radiative transfer

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1388:(LTE). It is important to note that local equilibrium may apply only to a certain subset of particles in the system. For example, LTE is usually applied only to massive particles. In a radiating gas, the photons being emitted and absorbed by the gas do not need to be in a thermodynamic equilibrium with each other or with the massive particles of the gas in order for LTE to exist. 67:). For a very small area element in the radiation field, there can be electromagnetic radiation passing in both senses in every spatial direction through it. In radiometric terms, the passage can be completely characterized by the amount of energy radiated in each of the two senses in each spatial direction, per unit time, per unit area of surface of sourcing passage, per unit 683: 1750: 903:
Solutions to the equation of radiative transfer form an enormous body of work. The differences however, are essentially due to the various forms for the emission and absorption coefficients. If scattering is ignored, then a general steady state solution in terms of the emission and absorption
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describes these interactions mathematically. Equations of radiative transfer have application in a wide variety of subjects including optics, astrophysics, atmospheric science, and remote sensing. Analytic solutions to the radiative transfer equation (RTE) exist for simple cases but for more
1113: 1395:). The radiation field is not, however in equilibrium and is being entirely driven by the presence of the massive particles. For a medium in LTE, the emission coefficient and absorption coefficient are functions of temperature and density only, and are related by: 1374: 2928: 462:
The equation of radiative transfer simply says that as a beam of radiation travels, it loses energy to absorption, gains energy by emission processes, and redistributes energy by scattering. The differential form of the equation for radiative transfer is:
2563: 1767:. The two-stream approximation assumes that the intensity is constant with angle in the upward hemisphere, with a different constant value in the downward hemisphere. The Eddington approximation instead assumes that the intensity is a linear function of 397: 2321:. Higher order versions of the Eddington approximation also exist, and consist of more complicated linear relations of the intensity moments. This extra equation can be used as a closure relation for the truncated system of moments. 2265: 2967: 2167: 2770: 678:{\displaystyle {\frac {1}{c}}{\frac {\partial }{\partial t}}I_{\nu }+{\hat {\Omega }}\cdot \nabla I_{\nu }+(k_{\nu ,s}+k_{\nu ,a})\rho I_{\nu }=j_{\nu }\rho +{\frac {1}{4\pi }}k_{\nu ,s}\rho \int _{\Omega }I_{\nu }d\Omega } 1972:. The Eddington approximation can be used to obtain the spectral radiance in a "plane-parallel" medium (one in which properties only vary in the perpendicular direction) with isotropic frequency-independent scattering. 1514: 893: 2655: 2076: 453:
makes with a normal to the area element. The units of the spectral radiance are seen to be energy/time/area/solid angle/frequency. In MKS units this would be W·m·sr·Hz (watts per square-metre-steradian-hertz).
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This equation shows how the effective optical depth in scattering-dominated systems may be significantly different from that given by the scattering opacity if the absorptive opacity is small.
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In this situation, the absorbing/emitting medium consists of massive particles which are locally in equilibrium with each other, and therefore have a definable temperature (
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realistic media, with complex multiple scattering effects, numerical methods are required. The present article is largely focused on the condition of
26:) is the physical phenomenon of energy transfer in the form of electromagnetic radiation. The propagation of radiation through a medium is affected by 2686: 1745:{\displaystyle I_{\nu }(s)=I_{\nu }(s_{0})e^{-\tau _{\nu }(s_{0},s)}+\int _{s_{0}}^{s}B_{\nu }(T(s'))\alpha _{\nu }(s')e^{-\tau _{\nu }(s',s)}\,ds'} 1755:
Knowing the temperature profile and the density profile of the medium is sufficient to calculate a solution to the equation of radiative transfer.
824: 2574: 2952: 2001: 1401: 2947: 1108:{\displaystyle I_{\nu }(s)=I_{\nu }(s_{0})e^{-\tau _{\nu }(s_{0},s)}+\int _{s_{0}}^{s}j_{\nu }(s')e^{-\tau _{\nu }(s',s)}\,ds'} 27: 3236: 3210: 3187: 3168: 3146: 3125: 3106: 3039: 3014: 31: 3286: 3136: 1369:{\displaystyle \tau _{\nu }(s_{1},s_{2})\ {\stackrel {\mathrm {def} }{=}}\ \int _{s_{1}}^{s_{2}}\alpha _{\nu }(s)\,ds} 3262: 3076: 1805: 3065:
Theory of Stellar Atmospheres, An Introduction to Astrophysical Non-equilibrium Quantitative Spectroscopic Analysis
2923:{\displaystyle {\frac {d^{2}J_{\nu }}{dz^{2}}}=3\alpha _{\nu }(\alpha _{\nu }+\sigma _{\nu })(J_{\nu }-B_{\nu })} 1965: 1923: 1385: 2558:{\displaystyle \mu {\frac {dI_{\nu }}{dz}}=-\alpha _{\nu }(I_{\nu }-B_{\nu })+\sigma _{\nu }(J_{\nu }-I_{\nu })} 3291: 1121: 392:{\displaystyle dE_{\nu }=I_{\nu }(\mathbf {r} ,{\hat {\mathbf {n} }},t)\cos \theta \ d\nu \,da\,d\Omega \,dt} 1392: 425: 201: 63: 2273: 1384:
A particularly useful simplification of the equation of radiative transfer occurs under the conditions of
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is the normal direction to the slab-like medium. Note that expressing angular integrals in terms of
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The radiative transfer through an isotropically scattering medium with scattering coefficient
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Radiative Transfer in Scattering and Absorbing Atmospheres: Standard Computational Procedures
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Radiative Transfer in Scattering and Absorbing Atmospheres: Standard Computational Procedures
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Radiative transfer equation and diffusion theory for photon transport in biological tissue
2663: 1978: 1903: 154: 108: 8: 3281: 2260:{\displaystyle K_{\nu }={\frac {1}{2}}\int _{-1}^{1}\mu ^{2}I_{\nu }d\mu ={\frac {a}{3}}} 3091: 2999: 2795:
allows the two above equations to be combined to form the radiative diffusion equation
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of reception at a distance, per unit wavelength interval being considered (
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Substituting in the closure relation, and differentiating with respect to
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Extracting the first few moments of the spectral radiance with respect to
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term represents radiation scattered from other directions onto a surface.
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Fundamentals of Atmospheric Radiation: an Introduction with 400 Problems
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The fundamental quantity that describes a field of radiation is called
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Note that the first two moments have simple physical meanings.
1508:. The solution to the equation of radiative transfer is then: 1454:{\displaystyle {\frac {j_{\nu }}{\alpha _{\nu }}}=B_{\nu }(T)} 3085: 3058: 2270:
Thus the Eddington approximation is equivalent to setting
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in radiometric terms (in other fields it is often called
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Energy transfer in the form of electromagnetic radiation
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Rybicki; Alan P. Lightman (1985). 2990: 2953:List of atmospheric radiative transfer codes 422:is the angle that the unit direction vector 3134: 2351:is the isotropic intensity at a point, and 1957:{\displaystyle d\mu =-\sin \theta d\theta } 3141:. Sundog Publishing (Madison, Wisconsin). 3219: 1730: 1359: 1167:{\displaystyle \tau _{\nu }(s_{1},s_{2})} 1093: 382: 375: 368: 269: 239: 164: 118: 3274: 3197:G. E. Thomas & K. Stamnes (1999). 3161:Foundations of Radiation Hydrodynamics 3023: 2378:is the flux through that point in the 3120:. A. Deepak Publishing. p. 583. 3034:. A. Deepak Publishing. p. 583. 446:{\displaystyle {\hat {\mathbf {n} }}} 222:{\displaystyle {\hat {\mathbf {n} }}} 2948:Kirchhoff's law of thermal radiation 2314:{\displaystyle K_{\nu }=1/3J_{\nu }} 3180:Radiative Processes in Astrophysics 2568:Integrating over all angles yields 78:In terms of the spectral radiance, 13: 3097:. Dover Publications Inc. p.  3052: 3005:. Dover Publications Inc. p.  1300: 1297: 1294: 882: 864: 672: 654: 526: 514: 489: 485: 458:The equation of radiative transfer 379: 185: 14: 3303: 3159:; Barbara Weibel-Mihalas (1984). 1792:{\displaystyle \mu =\cos \theta } 1504:spectral radiance at temperature 75:will be ignored for the moment). 1178:of the medium between positions 433: 331: 320: 209: 137: 3251:Principles of Planetary Climate 1386:local thermodynamic equilibrium 1380:Local thermodynamic equilibrium 2917: 2891: 2888: 2862: 2749: 2723: 2644: 2618: 2552: 2526: 2510: 2484: 2421:{\displaystyle \sigma _{\nu }} 1864: 1858: 1846: 1840: 1831: 1819: 1725: 1708: 1687: 1676: 1663: 1660: 1649: 1643: 1603: 1584: 1563: 1550: 1534: 1528: 1487: 1481: 1448: 1442: 1356: 1350: 1278: 1252: 1161: 1135: 1088: 1071: 1050: 1039: 999: 980: 959: 946: 930: 924: 580: 542: 517: 437: 347: 335: 316: 213: 50: 40:equation of radiative transfer 1: 2983: 904:coefficients may be written: 735:is the emission coefficient, 1393:Zeroth Law of Thermodynamics 821:is the mass density and the 273:{\displaystyle \nu +d\nu \,} 144:{\displaystyle \mathbf {r} } 7: 3163:. Dover Publications, Inc. 3116:Jacqueline Lenoble (1985). 3030:Jacqueline Lenoble (1985). 2936: 1759:The Eddington approximation 1493:{\displaystyle B_{\nu }(T)} 801:is the absorption opacity, 768:is the scattering opacity, 10: 3308: 3255:Cambridge University Press 3203:Cambridge University Press 3087:Subrahmanyan Chandrasekhar 3069:Princeton University Press 1920:simplifies things because 794:{\displaystyle k_{\nu ,a}} 761:{\displaystyle k_{\nu ,s}} 229:in the frequency interval 3287:Electromagnetic radiation 2997:S. Chandrasekhar (1960). 2978:Vector radiative transfer 2371:{\displaystyle H_{\nu }} 2344:{\displaystyle J_{\nu }} 1765:two-stream approximation 728:{\displaystyle j_{\nu }} 191:{\displaystyle d\Omega } 98:{\displaystyle I_{\nu }} 708:is the speed of light, 415:{\displaystyle \theta } 3182:. Wiley-Interscience. 2924: 2789: 2766: 2674: 2651: 2559: 2422: 2392: 2372: 2345: 2315: 2261: 2163: 2072: 1989: 1958: 1914: 1894: 1871: 1793: 1746: 1494: 1455: 1370: 1226: 1199: 1168: 1109: 889: 815: 795: 762: 729: 702: 679: 447: 416: 393: 274: 244: 243:{\displaystyle \nu \,} 223: 192: 169: 145: 123: 99: 3292:Atmospheric radiation 3229:John Wiley & Sons 2925: 2790: 2767: 2675: 2652: 2560: 2423: 2393: 2373: 2346: 2316: 2262: 2164: 2073: 1990: 1970:spherical coordinates 1959: 1915: 1895: 1872: 1794: 1747: 1495: 1456: 1371: 1227: 1225:{\displaystyle s_{2}} 1200: 1198:{\displaystyle s_{1}} 1169: 1110: 890: 816: 814:{\displaystyle \rho } 796: 763: 730: 703: 680: 448: 417: 394: 275: 245: 224: 193: 170: 146: 124: 100: 45:radiative equilibrium 3135:Grant Petty (2006). 2802: 2779: 2687: 2673:{\displaystyle \mu } 2664: 2575: 2435: 2405: 2382: 2355: 2328: 2274: 2174: 2083: 2002: 1988:{\displaystyle \mu } 1979: 1924: 1913:{\displaystyle \mu } 1904: 1884: 1806: 1771: 1515: 1468: 1402: 1239: 1209: 1182: 1122: 911: 825: 805: 772: 739: 712: 692: 470: 426: 406: 287: 254: 233: 202: 198:about the direction 179: 168:{\displaystyle dt\,} 155: 133: 122:{\displaystyle da\,} 109: 82: 3247:R. T. Pierrehumbert 2217: 2126: 2045: 1632: 1339: 1028: 175:in the solid angle 24:radiation transport 3093:Radiative Transfer 3001:Radiative Transfer 2920: 2785: 2762: 2670: 2660:Premultiplying by 2647: 2555: 2418: 2388: 2368: 2341: 2311: 2257: 2200: 2159: 2109: 2068: 2028: 1985: 1954: 1910: 1890: 1867: 1789: 1742: 1611: 1490: 1451: 1366: 1311: 1222: 1195: 1164: 1105: 1007: 885: 811: 791: 758: 725: 698: 675: 443: 412: 389: 270: 240: 219: 188: 165: 141: 119: 95: 64:specific intensity 20:Radiative transfer 3238:978-3-527-40503-9 3212:978-0-521-40124-1 3189:978-0-471-82759-7 3170:978-0-486-40925-2 3148:978-0-9729033-1-8 3127:978-0-12-451451-5 3108:978-0-486-60590-6 3041:978-0-12-451451-5 3016:978-0-486-60590-6 2844: 2788:{\displaystyle z} 2715: 2603: 2466: 2391:{\displaystyle z} 2255: 2198: 2157: 2107: 2026: 1893:{\displaystyle z} 1427: 1310: 1305: 1283: 841: 701:{\displaystyle c} 628: 520: 496: 481: 440: 361: 338: 216: 58:spectral radiance 3299: 3268: 3242: 3216: 3193: 3174: 3152: 3131: 3112: 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2039: 2027: 2019: 2014: 2013: 1994: 1992: 1991: 1986: 1968:of integrals in 1963: 1961: 1960: 1955: 1919: 1917: 1916: 1911: 1899: 1897: 1896: 1891: 1876: 1874: 1873: 1868: 1818: 1817: 1798: 1796: 1795: 1790: 1751: 1749: 1748: 1743: 1741: 1729: 1728: 1718: 1707: 1706: 1686: 1675: 1674: 1659: 1642: 1641: 1631: 1626: 1625: 1624: 1607: 1606: 1596: 1595: 1583: 1582: 1562: 1561: 1549: 1548: 1527: 1526: 1499: 1497: 1496: 1491: 1480: 1479: 1460: 1458: 1457: 1452: 1441: 1440: 1428: 1426: 1425: 1416: 1415: 1406: 1375: 1373: 1372: 1367: 1349: 1348: 1338: 1337: 1336: 1326: 1325: 1324: 1308: 1307: 1306: 1304: 1303: 1291: 1286: 1281: 1277: 1276: 1264: 1263: 1251: 1250: 1231: 1229: 1228: 1223: 1221: 1220: 1204: 1202: 1201: 1196: 1194: 1193: 1173: 1171: 1170: 1165: 1160: 1159: 1147: 1146: 1134: 1133: 1114: 1112: 1111: 1106: 1104: 1092: 1091: 1081: 1070: 1069: 1049: 1038: 1037: 1027: 1022: 1021: 1020: 1003: 1002: 992: 991: 979: 978: 958: 957: 945: 944: 923: 922: 894: 892: 891: 886: 878: 877: 868: 867: 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205: 203: 200: 199: 180: 177: 176: 156: 153: 152: 136: 134: 131: 130: 110: 107: 106: 89: 85: 83: 80: 79: 53: 38:processes. The 17: 12: 11: 5: 3305: 3295: 3294: 3289: 3284: 3270: 3269: 3263: 3243: 3237: 3217: 3211: 3194: 3188: 3175: 3169: 3153: 3147: 3132: 3126: 3113: 3107: 3083: 3077: 3054: 3051: 3048: 3047: 3040: 3022: 3015: 2988: 2987: 2985: 2982: 2981: 2980: 2975: 2970: 2965: 2960: 2955: 2950: 2945: 2938: 2935: 2931: 2930: 2919: 2914: 2910: 2906: 2901: 2897: 2893: 2890: 2885: 2881: 2877: 2872: 2868: 2864: 2859: 2855: 2851: 2848: 2840: 2836: 2832: 2825: 2821: 2815: 2811: 2784: 2773: 2772: 2759: 2755: 2751: 2746: 2742: 2738: 2733: 2729: 2725: 2722: 2719: 2713: 2710: 2703: 2699: 2695: 2669: 2658: 2657: 2646: 2641: 2637: 2633: 2628: 2624: 2620: 2615: 2611: 2607: 2601: 2598: 2591: 2587: 2583: 2566: 2565: 2554: 2549: 2545: 2541: 2536: 2532: 2528: 2523: 2519: 2515: 2512: 2507: 2503: 2499: 2494: 2490: 2486: 2481: 2477: 2473: 2470: 2464: 2461: 2454: 2450: 2446: 2440: 2415: 2411: 2387: 2365: 2361: 2338: 2334: 2308: 2304: 2300: 2296: 2292: 2289: 2284: 2280: 2268: 2267: 2254: 2251: 2246: 2243: 2240: 2235: 2231: 2225: 2221: 2215: 2210: 2207: 2203: 2197: 2194: 2189: 2184: 2180: 2169: 2156: 2153: 2148: 2145: 2142: 2137: 2133: 2129: 2124: 2119: 2116: 2112: 2106: 2103: 2098: 2093: 2089: 2078: 2067: 2064: 2061: 2058: 2053: 2049: 2043: 2038: 2035: 2031: 2025: 2022: 2017: 2012: 2008: 1984: 1953: 1950: 1947: 1944: 1941: 1938: 1935: 1932: 1929: 1909: 1889: 1878: 1877: 1866: 1863: 1860: 1857: 1854: 1851: 1848: 1845: 1842: 1839: 1836: 1833: 1830: 1827: 1824: 1821: 1816: 1812: 1788: 1785: 1782: 1779: 1776: 1760: 1757: 1753: 1752: 1740: 1737: 1733: 1727: 1724: 1721: 1717: 1714: 1710: 1705: 1701: 1697: 1693: 1689: 1685: 1682: 1678: 1673: 1669: 1665: 1662: 1658: 1655: 1651: 1648: 1645: 1640: 1636: 1630: 1623: 1619: 1614: 1610: 1605: 1602: 1599: 1594: 1590: 1586: 1581: 1577: 1573: 1569: 1565: 1560: 1556: 1552: 1547: 1543: 1539: 1536: 1533: 1530: 1525: 1521: 1489: 1486: 1483: 1478: 1474: 1462: 1461: 1450: 1447: 1444: 1439: 1435: 1431: 1424: 1420: 1414: 1410: 1381: 1378: 1377: 1376: 1365: 1362: 1358: 1355: 1352: 1347: 1343: 1335: 1331: 1323: 1319: 1314: 1302: 1299: 1296: 1290: 1280: 1275: 1271: 1267: 1262: 1258: 1254: 1249: 1245: 1219: 1215: 1192: 1188: 1163: 1158: 1154: 1150: 1145: 1141: 1137: 1132: 1128: 1116: 1115: 1103: 1100: 1096: 1090: 1087: 1084: 1080: 1077: 1073: 1068: 1064: 1060: 1056: 1052: 1048: 1045: 1041: 1036: 1032: 1026: 1019: 1015: 1010: 1006: 1001: 998: 995: 990: 986: 982: 977: 973: 969: 965: 961: 956: 952: 948: 943: 939: 935: 932: 929: 926: 921: 917: 900: 897: 884: 881: 876: 872: 866: 862: 856: 853: 850: 846: 839: 836: 832: 810: 788: 785: 782: 778: 755: 752: 749: 745: 722: 718: 697: 686: 685: 674: 671: 666: 662: 656: 652: 648: 643: 640: 637: 633: 626: 623: 619: 614: 611: 606: 602: 598: 593: 589: 585: 582: 577: 574: 571: 567: 563: 558: 555: 552: 548: 544: 541: 536: 532: 528: 525: 519: 516: 510: 505: 501: 494: 491: 487: 480: 477: 459: 456: 439: 435: 411: 400: 399: 388: 385: 381: 378: 374: 371: 367: 364: 358: 355: 352: 349: 346: 343: 337: 333: 326: 322: 318: 313: 309: 305: 300: 296: 292: 268: 265: 262: 259: 238: 215: 211: 187: 184: 163: 160: 139: 117: 114: 92: 88: 52: 49: 15: 9: 6: 4: 3: 2: 3304: 3293: 3290: 3288: 3285: 3283: 3280: 3279: 3277: 3266: 3264:9780521865562 3260: 3256: 3252: 3248: 3244: 3240: 3234: 3230: 3226: 3222: 3218: 3214: 3208: 3204: 3200: 3195: 3191: 3185: 3181: 3176: 3172: 3166: 3162: 3158: 3154: 3150: 3144: 3140: 3139: 3133: 3129: 3123: 3119: 3114: 3110: 3104: 3100: 3095: 3094: 3088: 3084: 3080: 3078:9780691163291 3074: 3070: 3066: 3062: 3059:Ivan Hubeny; 3057: 3056: 3043: 3037: 3033: 3026: 3018: 3012: 3008: 3003: 3002: 2993: 2989: 2979: 2976: 2974: 2971: 2969: 2966: 2964: 2961: 2959: 2958:Optical depth 2956: 2954: 2951: 2949: 2946: 2944: 2941: 2940: 2934: 2912: 2908: 2904: 2899: 2895: 2883: 2879: 2875: 2870: 2866: 2857: 2853: 2849: 2846: 2838: 2834: 2830: 2823: 2819: 2813: 2809: 2798: 2797: 2796: 2782: 2757: 2753: 2744: 2740: 2736: 2731: 2727: 2720: 2717: 2711: 2708: 2701: 2697: 2693: 2683: 2682: 2681: 2667: 2639: 2635: 2631: 2626: 2622: 2613: 2609: 2605: 2599: 2596: 2589: 2585: 2581: 2571: 2570: 2569: 2547: 2543: 2539: 2534: 2530: 2521: 2517: 2513: 2505: 2501: 2497: 2492: 2488: 2479: 2475: 2471: 2468: 2462: 2459: 2452: 2448: 2444: 2438: 2431: 2430: 2429: 2413: 2409: 2399: 2385: 2363: 2359: 2336: 2332: 2322: 2306: 2302: 2298: 2294: 2290: 2287: 2282: 2278: 2252: 2249: 2244: 2241: 2238: 2233: 2229: 2223: 2219: 2213: 2208: 2205: 2201: 2195: 2192: 2187: 2182: 2178: 2170: 2154: 2151: 2146: 2143: 2140: 2135: 2131: 2127: 2122: 2117: 2114: 2110: 2104: 2101: 2096: 2091: 2087: 2079: 2065: 2062: 2059: 2056: 2051: 2047: 2041: 2036: 2033: 2029: 2023: 2020: 2015: 2010: 2006: 1998: 1997: 1996: 1982: 1973: 1971: 1967: 1951: 1948: 1945: 1942: 1939: 1936: 1933: 1930: 1927: 1907: 1887: 1861: 1855: 1852: 1849: 1843: 1837: 1834: 1828: 1825: 1822: 1814: 1810: 1802: 1801: 1800: 1786: 1783: 1780: 1777: 1774: 1766: 1756: 1738: 1735: 1731: 1722: 1719: 1715: 1712: 1703: 1699: 1695: 1691: 1683: 1680: 1671: 1667: 1656: 1653: 1646: 1638: 1634: 1628: 1621: 1617: 1612: 1608: 1600: 1597: 1592: 1588: 1579: 1575: 1571: 1567: 1558: 1554: 1545: 1541: 1537: 1531: 1523: 1519: 1511: 1510: 1509: 1507: 1503: 1484: 1476: 1472: 1445: 1437: 1433: 1429: 1422: 1418: 1412: 1408: 1398: 1397: 1396: 1394: 1389: 1387: 1363: 1360: 1353: 1345: 1341: 1333: 1329: 1321: 1317: 1312: 1288: 1273: 1269: 1265: 1260: 1256: 1247: 1243: 1235: 1234: 1233: 1217: 1213: 1190: 1186: 1177: 1176:optical depth 1156: 1152: 1148: 1143: 1139: 1130: 1126: 1101: 1098: 1094: 1085: 1082: 1078: 1075: 1066: 1062: 1058: 1054: 1046: 1043: 1034: 1030: 1024: 1017: 1013: 1008: 1004: 996: 993: 988: 984: 975: 971: 967: 963: 954: 950: 941: 937: 933: 927: 919: 915: 907: 906: 905: 896: 879: 874: 870: 860: 854: 851: 848: 844: 837: 834: 830: 808: 786: 783: 780: 776: 753: 750: 747: 743: 720: 716: 695: 669: 664: 660: 650: 646: 641: 638: 635: 631: 624: 621: 617: 612: 609: 604: 600: 596: 591: 587: 583: 575: 572: 569: 565: 561: 556: 553: 550: 546: 539: 534: 530: 523: 508: 503: 499: 492: 478: 475: 466: 465: 464: 455: 409: 386: 383: 376: 372: 369: 365: 362: 356: 353: 350: 344: 341: 324: 311: 307: 303: 298: 294: 290: 283: 282: 281: 266: 263: 260: 257: 236: 182: 161: 158: 115: 112: 90: 86: 76: 74: 70: 66: 65: 60: 59: 48: 46: 41: 37: 33: 29: 25: 22:(also called 21: 3250: 3224: 3198: 3179: 3160: 3137: 3117: 3092: 3064: 3031: 3025: 3000: 2992: 2963:Planck's law 2932: 2774: 2659: 2567: 2400: 2323: 2269: 1974: 1879: 1762: 1754: 1505: 1463: 1390: 1383: 1117: 902: 687: 461: 401: 77: 73:polarization 62: 56: 54: 39: 23: 19: 18: 2398:direction. 129:located at 69:solid angle 51:Definitions 3282:Radiometry 3276:Categories 2984:References 1502:black body 36:scattering 28:absorption 3221:C. Bohren 2913:ν 2905:− 2900:ν 2884:ν 2880:σ 2871:ν 2867:α 2858:ν 2854:α 2824:ν 2758:ν 2745:ν 2741:σ 2732:ν 2728:α 2721:− 2702:ν 2668:μ 2640:ν 2632:− 2627:ν 2614:ν 2610:α 2590:ν 2548:ν 2540:− 2535:ν 2522:ν 2518:σ 2506:ν 2498:− 2493:ν 2480:ν 2476:α 2472:− 2453:ν 2439:μ 2414:ν 2410:σ 2364:ν 2337:ν 2307:ν 2283:ν 2242:μ 2234:ν 2220:μ 2206:− 2202:∫ 2183:ν 2144:μ 2136:ν 2128:μ 2115:− 2111:∫ 2092:ν 2060:μ 2052:ν 2034:− 2030:∫ 2011:ν 1983:μ 1952:θ 1946:θ 1943:⁡ 1937:− 1931:μ 1908:μ 1853:μ 1823:μ 1815:ν 1787:θ 1784:⁡ 1775:μ 1704:ν 1700:τ 1696:− 1672:ν 1668:α 1639:ν 1613:∫ 1580:ν 1576:τ 1572:− 1546:ν 1524:ν 1477:ν 1438:ν 1423:ν 1419:α 1413:ν 1346:ν 1342:α 1313:∫ 1248:ν 1244:τ 1131:ν 1127:τ 1067:ν 1063:τ 1059:− 1035:ν 1009:∫ 976:ν 972:τ 968:− 942:ν 920:ν 883:Ω 875:ν 865:Ω 861:∫ 849:ν 838:π 809:ρ 781:ν 748:ν 721:ν 673:Ω 665:ν 655:Ω 651:∫ 647:ρ 636:ν 625:π 610:ρ 605:ν 592:ν 584:ρ 570:ν 551:ν 535:ν 527:∇ 524:⋅ 518:^ 515:Ω 504:ν 490:∂ 486:∂ 438:^ 410:θ 380:Ω 366:ν 357:θ 354:⁡ 336:^ 312:ν 299:ν 267:ν 258:ν 237:ν 214:^ 186:Ω 91:ν 3249:(2010). 3223:(2006). 3089:(1960). 3063:(2015). 2937:See also 1966:Jacobian 1739:′ 1716:′ 1684:′ 1657:′ 1102:′ 1079:′ 1047:′ 151:in time 32:emission 1995:yields 1799:, i.e. 1500:is the 1174:is the 3261:  3235:  3209:  3186:  3167:  3145:  3124:  3105:  3075:  3038:  3013:  1880:where 1464:where 1309:  1282:  1118:where 688:where 402:where 360:  34:, and 3259:ISBN 3233:ISBN 3207:ISBN 3184:ISBN 3165:ISBN 3143:ISBN 3122:ISBN 3103:ISBN 3073:ISBN 3036:ISBN 3011:ISBN 1205:and 3099:393 3007:393 1940:sin 1781:cos 351:cos 280:is 250:to 3278:: 3257:. 3253:. 3231:. 3227:. 3205:. 3201:. 3101:. 3067:. 3009:. 1232:: 47:. 30:, 3267:. 3241:. 3215:. 3192:. 3173:. 3151:. 3130:. 3111:. 3081:. 3044:. 3019:. 2918:) 2909:B 2896:J 2892:( 2889:) 2876:+ 2863:( 2850:3 2847:= 2839:2 2835:z 2831:d 2820:J 2814:2 2810:d 2783:z 2754:H 2750:) 2737:+ 2724:( 2718:= 2712:z 2709:d 2698:K 2694:d 2645:) 2636:J 2623:B 2619:( 2606:= 2600:z 2597:d 2586:H 2582:d 2553:) 2544:I 2531:J 2527:( 2514:+ 2511:) 2502:B 2489:I 2485:( 2469:= 2463:z 2460:d 2449:I 2445:d 2386:z 2360:H 2333:J 2303:J 2299:3 2295:/ 2291:1 2288:= 2279:K 2253:3 2250:a 2245:= 2239:d 2230:I 2224:2 2214:1 2209:1 2196:2 2193:1 2188:= 2179:K 2155:3 2152:b 2147:= 2141:d 2132:I 2123:1 2118:1 2105:2 2102:1 2097:= 2088:H 2066:a 2063:= 2057:d 2048:I 2042:1 2037:1 2024:2 2021:1 2016:= 2007:J 1949:d 1934:= 1928:d 1888:z 1865:) 1862:z 1859:( 1856:b 1850:+ 1847:) 1844:z 1841:( 1838:a 1835:= 1832:) 1829:z 1826:, 1820:( 1811:I 1778:= 1736:s 1732:d 1726:) 1723:s 1720:, 1713:s 1709:( 1692:e 1688:) 1681:s 1677:( 1664:) 1661:) 1654:s 1650:( 1647:T 1644:( 1635:B 1629:s 1622:0 1618:s 1609:+ 1604:) 1601:s 1598:, 1593:0 1589:s 1585:( 1568:e 1564:) 1559:0 1555:s 1551:( 1542:I 1538:= 1535:) 1532:s 1529:( 1520:I 1506:T 1488:) 1485:T 1482:( 1473:B 1449:) 1446:T 1443:( 1434:B 1430:= 1409:j 1364:s 1361:d 1357:) 1354:s 1351:( 1334:2 1330:s 1322:1 1318:s 1301:f 1298:e 1295:d 1289:= 1279:) 1274:2 1270:s 1266:, 1261:1 1257:s 1253:( 1218:2 1214:s 1191:1 1187:s 1162:) 1157:2 1153:s 1149:, 1144:1 1140:s 1136:( 1099:s 1095:d 1089:) 1086:s 1083:, 1076:s 1072:( 1055:e 1051:) 1044:s 1040:( 1031:j 1025:s 1018:0 1014:s 1005:+ 1000:) 997:s 994:, 989:0 985:s 981:( 964:e 960:) 955:0 951:s 947:( 938:I 934:= 931:) 928:s 925:( 916:I 880:d 871:I 855:s 852:, 845:k 835:4 831:1 787:a 784:, 777:k 754:s 751:, 744:k 717:j 696:c 670:d 661:I 642:s 639:, 632:k 622:4 618:1 613:+ 601:j 597:= 588:I 581:) 576:a 573:, 566:k 562:+ 557:s 554:, 547:k 543:( 540:+ 531:I 509:+ 500:I 493:t 479:c 476:1 434:n 387:t 384:d 377:d 373:a 370:d 363:d 348:) 345:t 342:, 332:n 325:, 321:r 317:( 308:I 304:= 295:E 291:d 264:d 261:+ 210:n 183:d 162:t 159:d 138:r 116:a 113:d 87:I

Index

absorption
emission
scattering
radiative equilibrium
spectral radiance
specific intensity
solid angle
polarization
optical depth
local thermodynamic equilibrium
Zeroth Law of Thermodynamics
black body
two-stream approximation
Jacobian
spherical coordinates
Beer-Lambert law
Kirchhoff's law of thermal radiation
List of atmospheric radiative transfer codes
Optical depth
Planck's law
Radiative transfer equation and diffusion theory for photon transport in biological tissue
Schwarzschild's equation for radiative transfer
Vector radiative transfer
Radiative Transfer
393
ISBN
978-0-486-60590-6
ISBN
978-0-12-451451-5
Dimitri Mihalas

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