1886:
535:
430:
233:
630:
1550:
per unit frequency or wavelength. The latter is commonly measured in W⋅m⋅nm. "Spectral emittance" is an old term for this quantity. This is sometimes also confusingly called "spectral intensity".
659:
Unlike power density, radiant intensity does not depend on distance: because radiant intensity is defined as the power through a solid angle, the decreasing power density over distance due to the
458:
353:
168:
1508:
per unit area. This is the emitted component of radiosity. "Radiant emittance" is an old term for this quantity. This is sometimes also confusingly called "intensity".
1937:
695:
1284:
per unit frequency or wavelength. This is sometimes also confusingly called "spectral intensity". Non-SI units of spectral flux density include
1431:
per unit frequency or wavelength. The latter is commonly measured in W⋅m⋅nm. This is sometimes also confusingly called "spectral intensity".
562:
855:
Radiant energy emitted, reflected, transmitted or received, per unit time. This is sometimes also called "radiant power", and called
1967:
688:
35:
1986:
1669:
per unit frequency or wavelength. The latter is commonly measured in J⋅m⋅nm. This is sometimes also called "spectral fluence".
78:
70:
2002:
681:
128:
1929:
530:{\displaystyle I_{\mathrm {e} ,\Omega ,\lambda }={\frac {\partial I_{\mathrm {e} ,\Omega }}{\partial \lambda }},}
325:
refers to the solid angle into which the light is emitted. When calculating radiance received by a detector,
298:
1741:
1394:
1351:
1028:
Radiant intensity per unit frequency or wavelength. The latter is commonly measured in W⋅sr⋅nm. This is a
779:
287:
425:{\displaystyle I_{\mathrm {e} ,\Omega ,\nu }={\frac {\partial I_{\mathrm {e} ,\Omega }}{\partial \nu }},}
1247:
158:("e" for "energetic", to avoid confusion with photometric quantities, and "Ω" to indicate this is a
2007:
1722:
228:{\displaystyle I_{\mathrm {e} ,\Omega }={\frac {\partial \Phi _{\mathrm {e} }}{\partial \Omega }},}
119:
1904:
660:
243:
1963:
1885:
1745:
1114:
1632:
1589:
1513:
1470:
114:
1748:
should be denoted with suffix "e" (for "energetic") to avoid confusion with photometric or
1297:
1153:
per unit frequency or wavelength. The latter is commonly measured in W⋅sr⋅m⋅nm. This is a
982:
Radiant flux emitted, reflected, transmitted or received, per unit solid angle. This is a
553:
905:
Radiant flux per unit frequency or wavelength. The latter is commonly measured in W⋅nm.
1930:"Thermal insulation — Heat transfer by radiation — Physical quantities and definitions"
736:
31:
1627:
integrated over time of irradiation. This is sometimes also called "radiant fluence".
1996:
283:
101:) and that of spectral intensity in wavelength is the watt per steradian per metre (
1200:
864:
818:
254:
50:
17:
1827:
329:
refers to the solid angle subtended by the source as viewed from that detector.
264:
54:
93:), while that of spectral intensity in frequency is the watt per steradian per
1853:
1717:
1243:
1196:
856:
646:
110:
66:
42:
1817:
964:
958:
86:
62:
1830:, not to be confused with a letter "v", indicating a photometric quantity.)
1157:
quantity. This is sometimes also confusingly called "spectral intensity".
552:
Radiant intensity is used to characterize the emission of radiation by an
1071:
1899:
124:
1389:
per unit area. This is sometimes also confusingly called "intensity".
1238:
per unit area. This is sometimes also confusingly called "intensity".
1766:
1764:
1762:
1760:
1758:
1749:
1285:
625:{\displaystyle I_{\mathrm {e} ,\Omega }=E_{\mathrm {e} }(r)\,r^{2},}
1884:
887:
881:
756:
751:
94:
30:"Radiation intensity" redirects here. For ionizing radiation, see
1109:
quantity. This is sometimes also confusingly called "intensity".
1875:
1858:
1822:
836:
831:
82:
73:
is taken as a function of frequency or of wavelength. These are
1101:
Radiant flux emitted, reflected, transmitted or received by a
321:
When calculating the radiant intensity emitted by a source,
1712:
1105:, per unit solid angle per unit projected area. This is a
34:. For other measures of electromagnetic radiation, see
53:
emitted, reflected, transmitted or received, per unit
565:
461:
356:
171:
1889:
Comparison of photometric and radiometric quantities
1848:
1846:
1844:
1842:
1840:
1838:
1836:
1870:
1868:
624:
529:
424:
227:
663:is offset by the increase in area with distance.
105:)—commonly the watt per steradian per nanometre (
1874:Directional quantities are denoted with suffix "
1812:
1810:
1808:
1806:
1804:
1802:
1800:
1924:
1922:
1920:
1623:per unit area, or equivalently irradiance of a
1175:watt per steradian per square metre, per metre
1134:watt per steradian per square metre per hertz
689:
8:
1958:de Kraus, John; Marhefka, Ronald J. (2002).
257:emitted, reflected, transmitted or received;
1385:(emitted, reflected and transmitted by) a
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682:
672:
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204:
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193:
177:
176:
170:
131:, radiant intensity is sometimes called
1916:
1734:
109:). Radiant intensity is distinct from
27:Intensity of electromagnetic radiation
1631:
1512:
1393:
1242:
1113:
990:
863:
774:Energy of electromagnetic radiation.
716:
713:
710:
707:
7:
1770:Alternative symbols sometimes seen:
1086:watt per steradian per square metre
1852:Spectral quantities given per unit
1816:Spectral quantities given per unit
1687:joule per square metre, per metre
593:
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403:
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216:
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205:
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196:
185:
178:
61:is the radiant intensity per unit
25:
1987:Radiation: Activity and Intensity
1650:joule per square metre per hertz
1568:watt per square metre, per metre
1449:watt per square metre, per metre
1330:watt per square metre, per metre
655:is the distance from the antenna.
1531:watt per square metre per hertz
1412:watt per square metre per hertz
1265:watt per square metre per hertz
813:Radiant energy per unit volume.
443:Spectral intensity in wavelength
36:Light intensity (disambiguation)
338:Spectral intensity in frequency
278:is a function of viewing angle
605:
599:
1:
1960:Antennas for all applications
1619:Radiant energy received by a
1050:watt per steradian per metre
1009:watt per steradian per hertz
286:. For the special case of a
81:of radiant intensity is the
1744:recommend that radiometric
548:Radio-frequency engineering
129:radio-frequency engineering
69:, depending on whether the
2024:
127:other than radiometry. In
29:
1856:are denoted with suffix "
1820:are denoted with suffix "
1707:
1664:
1588:
1545:
1469:
1426:
1350:
1279:
1195:
1148:
1070:
1027:
941:
904:
817:
778:
735:
730:
727:
724:
721:
162:quantity), is defined as
117:, which are often called
139:Mathematical definitions
1989:NDE/NDT Resource Center
1742:Standards organizations
1604:joule per square metre
1890:
1665:Radiant exposure of a
1546:Radiant exitance of a
1485:watt per square metre
1366:watt per square metre
1215:watt per square metre
794:joule per cubic metre
780:Radiant energy density
626:
531:
426:
229:
1888:
1794:for radiant exitance.
1248:Spectral flux density
627:
532:
427:
230:
1778:for radiant energy,
563:
459:
354:
299:Lambert's cosine law
169:
2003:Physical quantities
1244:Spectral irradiance
1118:Specific intensity
704:
676:SI radiometry units
667:SI radiometry units
544:is the wavelength.
133:radiation intensity
18:Radiation intensity
1905:Luminous intensity
1891:
1786:for radiant flux,
1395:Spectral radiosity
992:Spectral intensity
673:
661:inverse-square law
622:
527:
439:is the frequency.
422:
333:Spectral intensity
288:Lambertian surface
244:partial derivative
225:
59:spectral intensity
1731:
1730:
1633:Spectral exposure
1514:Spectral exitance
1115:Spectral radiance
943:Radiant intensity
522:
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220:
149:Radiant intensity
144:Radiant intensity
47:radiant intensity
16:(Redirected from
2015:
1974:
1973:
1962:(3rd ed.).
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1826:" (Greek letter
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77:quantities. The
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1427:Radiosity of a
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1298:solar flux unit
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1130:
1121:
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921:watt per metre
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123:in branches of
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1981:External links
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1459:
1455:
1442:
1437:
1428:
1422:
1418:
1405:
1400:
1386:
1382:
1376:
1372:
1357:
1344:
1340:
1336:
1323:
1318:
1281:
1275:
1271:
1258:
1253:
1235:
1231:
1225:
1221:
1206:
1201:Flux density
1189:
1185:
1181:
1168:
1163:
1154:
1150:
1144:
1140:
1127:
1122:
1106:
1102:
1096:
1092:
1077:
1064:
1060:
1056:
1043:
1038:
1029:
1023:
1019:
1015:
1002:
997:
991:
983:
977:
973:
969:
948:
942:
935:
931:
927:
914:
900:
896:
892:
873:
850:
846:
842:
819:Radiant flux
808:
804:
800:
785:
769:
765:
761:
742:
670:
658:
652:
639:
634:
551:
541:
539:
446:
442:
441:
436:
434:
341:
337:
336:
326:
322:
320:
315:
308:
301:
297:follows the
291:
279:
272:
271:In general,
270:
260:
255:radiant flux
237:
159:
152:
148:
147:
132:
118:
74:
58:
51:radiant flux
46:
40:
1752:quantities.
1155:directional
1107:directional
1030:directional
984:directional
265:solid angle
160:directional
75:directional
55:solid angle
2008:Radiometry
1997:Categories
1944:2015-03-15
1911:References
1854:wavelength
1746:quantities
1723:Photometry
1718:Radiometry
1708:See also:
1310:10 Jy
1302:1 sfu
1197:Irradiance
1137:W⋅sr⋅m⋅Hz
1032:quantity.
986:quantity.
857:luminosity
714:Dimension
647:irradiance
445:, denoted
340:, denoted
151:, denoted
111:irradiance
67:wavelength
43:radiometry
1818:frequency
1352:Radiosity
1290:1 Jy
959:steradian
957:watt per
880:watt per
708:Quantity
580:Ω
519:λ
516:∂
509:Ω
493:∂
482:λ
476:Ω
414:ν
411:∂
404:Ω
388:∂
377:ν
371:Ω
242:∂ is the
217:Ω
214:∂
201:Φ
197:∂
186:Ω
120:intensity
87:steradian
63:frequency
1894:See also
1232:received
1072:Radiance
1012:W⋅sr⋅Hz
71:spectrum
1900:Candela
1667:surface
1653:J⋅m⋅Hz
1625:surface
1621:surface
1548:surface
1534:W⋅m⋅Hz
1506:surface
1502:emitted
1429:surface
1415:W⋅m⋅Hz
1387:surface
1383:leaving
1282:surface
1268:W⋅m⋅Hz
1236:surface
1178:W⋅sr⋅m
1151:surface
1103:surface
1089:W⋅sr⋅m
1053:W⋅sr⋅m
731:Symbol
725:Symbol
645:is the
554:antenna
263:is the
253:is the
246:symbol;
125:physics
107:W·sr·nm
99:W·sr·Hz
79:SI unit
49:is the
1966:
1750:photon
1296:) and
1286:jansky
839:= J/s
717:Notes
635:where
540:where
435:where
238:where
103:W·sr·m
57:, and
1504:by a
1234:by a
882:hertz
752:joule
728:Name
722:Name
711:Unit
450:e,Ω,λ
345:e,Ω,ν
95:hertz
1964:ISBN
1690:J/m
1607:J/m
1571:W/m
1488:W/m
1452:W/m
1369:W/m
1333:W/m
1218:W/m
1167:e,Ω,
1126:e,Ω,
1042:e,Ω,
1001:e,Ω,
924:W/m
832:watt
797:J/m
314:cos
113:and
91:W/sr
85:per
83:watt
1938:ISO
1782:or
1774:or
1312:).
1081:e,Ω
952:e,Ω
305:e,Ω
295:e,Ω
276:e,Ω
156:e,Ω
65:or
41:In
1999::
1936:.
1932:.
1919:^
1878:".
1867:^
1862:".
1835:^
1828:nu
1799:^
1757:^
1713:SI
1679:e,
1642:e,
1560:e,
1523:e,
1441:e,
1404:e,
1322:e,
1308:=
1304:=
1292:=
1257:e,
965:sr
963:W/
913:e,
888:Hz
886:W/
872:e,
556::
318:.
307:=
290:,
135:.
45:,
1972:.
1947:.
1876:Ω
1859:λ
1823:ν
1792:W
1788:I
1784:F
1780:P
1776:E
1772:W
1702:T
1700:⋅
1698:L
1696:⋅
1694:M
1681:λ
1676:H
1661:T
1659:⋅
1657:M
1644:ν
1639:H
1615:T
1613:⋅
1611:M
1599:e
1596:H
1583:T
1581:⋅
1579:L
1577:⋅
1575:M
1562:λ
1557:M
1542:T
1540:⋅
1538:M
1525:ν
1520:M
1496:T
1494:⋅
1492:M
1480:e
1477:M
1464:T
1462:⋅
1460:L
1458:⋅
1456:M
1443:λ
1438:J
1423:T
1421:⋅
1419:M
1406:ν
1401:J
1377:T
1375:⋅
1373:M
1361:e
1358:J
1345:T
1343:⋅
1341:L
1339:⋅
1337:M
1324:λ
1319:E
1300:(
1288:(
1276:T
1274:⋅
1272:M
1259:ν
1254:E
1226:T
1224:⋅
1222:M
1210:e
1207:E
1190:T
1188:⋅
1186:L
1184:⋅
1182:M
1169:λ
1164:L
1145:T
1143:⋅
1141:M
1128:ν
1123:L
1097:T
1095:⋅
1093:M
1078:L
1065:T
1063:⋅
1061:L
1059:⋅
1057:M
1044:λ
1039:I
1024:T
1022:⋅
1020:L
1018:⋅
1016:M
1003:ν
998:I
978:T
976:⋅
974:L
972:⋅
970:M
949:I
936:T
934:⋅
932:L
930:⋅
928:M
915:λ
911:Φ
901:T
899:⋅
897:L
895:⋅
893:M
874:ν
870:Φ
851:T
849:⋅
847:L
845:⋅
843:M
837:W
826:e
824:Φ
809:T
807:⋅
805:L
803:⋅
801:M
789:e
786:w
770:T
768:⋅
766:L
764:⋅
762:M
757:J
746:e
743:Q
697:e
690:t
683:v
653:r
643:e
640:E
620:,
615:2
611:r
606:)
603:r
600:(
594:e
589:E
585:=
577:,
573:e
568:I
542:λ
525:,
506:,
502:e
497:I
487:=
479:,
473:,
469:e
464:I
447:I
437:ν
420:,
401:,
397:e
392:I
382:=
374:,
368:,
364:e
359:I
342:I
327:Ω
323:Ω
316:θ
312:0
309:I
302:I
292:I
280:θ
273:I
267:.
261:Ω
251:e
249:Φ
223:,
206:e
191:=
183:,
179:e
174:I
153:I
97:(
89:(
38:.
20:)
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