Knowledge (XXG)

Gloss (optics)

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If black and white surfaces of the same shininess are visually compared, the black surface will always appear glossier because of the greater contrast between the specular highlight and the black surroundings as compared to that with white surface and surroundings. Pfund was also the first to suggest
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In the 1930s work by A. H. Pfund, suggested that although specular shininess is the basic (objective) evidence of gloss, actual surface glossy appearance (subjective) relates to the contrast between specular shininess and the diffuse light of the surrounding surface area (now called "contrast gloss"
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Studies of polished metal surfaces and anodised aluminium automotive trim in the 1960s by Tingle, Potter and George led to the standardisation of gloss measurement of high gloss surfaces by goniophotometry under the designation ASTM E430. In this standard it also defined methods for the measurement
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Substrate material type also influences the gloss of a surface. Non-metallic materials, i.e. plastics etc. produce a higher level of reflected light when illuminated at a greater illumination angle due to light being absorbed into the material or being diffusely scattered depending on the colour of
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The earliest studies of gloss perception are attributed to Ingersoll who in 1914 examined the effect of gloss on paper. By quantitatively measuring gloss using instrumentation Ingersoll based his research around the theory that light is polarised in specular reflection whereas diffusely reflected
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Variations in surface texture directly influence the level of specular reflection. Objects with a smooth surface, i.e. highly polished or containing coatings with finely dispersed pigments, appear shiny to the eye due to a large amount of light being reflected in a specular direction whilst rough
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with a specular angle of 45° as did most of the first photoelectric methods of that type, later studies however by Hunter and Judd in 1939, on a larger number of painted samples, concluded that the 60 degree geometry was the best angle to use so as to provide the closest correlation to a visual
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In the paint industry, measurements of the specular gloss are made according to International Standard ISO 2813 (BS 3900, Part 5, UK; DIN 67530, Germany; NFT 30-064, France; AS 1580, Australia; JIS Z8741, Japan, are also equivalent). This standard is essentially the same as ASTM D523 although
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Standardisation in gloss measurement was led by Hunter and ASTM (American Society for Testing and Materials) who produced ASTM D523 Standard test method for specular gloss in 1939. This incorporated a method for measuring gloss at a specular angle of 60°. Later editions of the Standard (1951)
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A surface can therefore appear very shiny if it has a well-defined specular reflectance at the specular angle. The perception of an image reflected in the surface can be degraded by appearing unsharp, or by appearing to be of low contrast. The former is characterised by the measurement of the
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In 1937 Hunter, as part of his research paper on gloss, described six different visual criteria attributed to apparent gloss. The following diagrams show the relationships between an incident beam of light, I, a specularly reflected beam, S, a diffusely reflected beam, D and a near-specularly
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light is non-polarized. The Ingersoll "glarimeter" had a specular geometry with incident and viewing angles at 57.5°. Using this configuration gloss was measured using a contrast method which subtracted the specular component from the total reflectance using a polarizing filter.
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In 1937, the paper industry adopted a 75° specular-gloss method because the angle gave the best separation of coated book papers. This method was adopted in 1951 by the Technical Association of Pulp and Paper Industries as TAPPI Method T480.
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surfaces reflect no specular light as the light is scattered in other directions and therefore appears dull. The image forming qualities of these surfaces are much lower making any reflections appear blurred and distorted.
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ASTM has a number of other gloss-related standards designed for application in specific industries including the old 45° method which is used primarily now used for glazed ceramics, polyethylene and other plastic films.
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in an order system with three variables, including gloss among the involved aspects. The factors that affect gloss are the refractive index of the material, the angle of incident light and the
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of an object. Other categories of visual appearance related to the perception of regular or diffuse reflection and transmission of light have been organized under the concept of
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Tingle, W. H., and George, D. J., “Measuring Appearance Characteristics of Anodized Aluminum Automotive Trim,” Report No. 650513, Society of Automotive Engineers, May 1965.
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included methods for measuring at 20° for evaluating high gloss finishes, developed at the DuPont Company (Horning and Morse, 1947) and 85° (matte, or low, gloss).
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Defined as a measure of the absence of haze or a milky appearance adjacent to the specularly reflected light: haze is the inverse of absence-of-bloom
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reflection – light reflected from the surface in an equal amount and the symmetrical angle to the one of incoming light – in comparison with
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Ingersoll Elec. World 63,645 (1914), Elec. World 64, 35 (1915); Paper 27, 18 (Feb. 9, 1921), and U. S. Patent 1225250 (May 8, 1917)
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Tingle, W. H., and Potter, F. R., “New Instrument Grades for Polished Metal Surfaces,” Product Engineering, Vol 27, March 1961.
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Defined as the uniformity of the surface in terms of visible texture and defects (orange peel, scratches, inclusions etc.)
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Defined as the ratio of the light reflected from a surface at an equal but opposite angle to that incident on the surface.
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Ingersoll R. S., The Glarimeter, "An instrument for measuring the gloss of paper". J.Opt. Soc. Am. 5.213 (1921)
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Defined as the ratio of the specularly reflected light to that diffusely reflected normal to the surface;
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the material. Metals do not suffer from this effect producing higher amounts of reflection at any angle.
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In his paper Hunter also noted the importance of three main factors in the measurement of gloss:
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Surface roughness influences the specular reflectance levels; in the visible frequencies, the
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Optical property describing the ability of a surface to reflect light in a specular direction
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Distinctness of image gloss – identified by the distinctness of images reflected in surfaces
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Surface texture gloss – identified by the lack of surface texture and surface blemishes
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Absence of bloom – the perceived cloudiness in reflections near the specular direction
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Contrast gloss – the perceived brightness of specularly and diffusely reflecting areas
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range is most relevant. The diagram on the right depicts the reflection at an angle
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Hunter, R. S., "Methods of determining gloss", RP958 J. Res. NBS, Volume 18 (1937)
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The amount and way in which the light is spread around the specular direction
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When light illuminates an object, it interacts with it in a number of ways:
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A. H. Pfund, "The measurement of gloss", J. Opt. Soc. Am. 20, 23.23 (1930)
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Specular gloss – the perceived brightness and the brilliance of highlights
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Transmitted through it (dependent on the surface transparency and opacity)
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is small, the two beams (see Figure 1) are nearly in phase, resulting in
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PCI Magazin article: What is the Level of Confidence in Measuring Gloss?
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Scattered from or within it (diffuse reflection, haze and transmission)
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Judd, D B (1937), Gloss and glossiness. Am. Dyest. Rep. 26, 234–235
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distinctness-of-image and the latter by the haze or contrast gloss.
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on a rough surface with a characteristic roughness height variation
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that more than one method was needed to analyze gloss correctly.
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Defined as the gloss at grazing angles of incidence and viewing
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property which indicates how well a surface reflects light in a
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The change in specular reflection as the specular angle changes
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Defined as the sharpness of the specularly reflected light
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Figure1: Specular reflection of light from a rough surface
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The amount of light reflected in the specular direction
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NPL: Good practice guide for the measurement of Gloss
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Sheen – the perceived shininess at low grazing angles
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of distinctness of image gloss and reflection haze.
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The Fresnel formula gives the specular reflectance,
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Absorbed within it (largely responsible for colour)
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"Part 10". 1104: 1082: 1067: 1052: 1037: 1022: 749:, the phase difference will be: 96:Specular and diffuse reflection 1286:Optical Properties of Polymers 853:{\displaystyle \Delta \phi \;} 152:, for an unpolarized light of 1: 1265:Paint and Coating Test Manual 991:Rayleigh roughness criterion 1125:For his research he used a 256:is given as follows : 18:Gloss (material appearance) 1351: 1134:Standard gloss measurement 29: 862:constructive interference 896:destructive interference 742:{\displaystyle \lambda } 671:{\displaystyle \Delta h} 182:, at angle of incidence 1165:List of optical topics 1151:differently drafted. 980: 929: 888: 854: 827: 743: 720: 672: 649: 624: 605: 304: 243: 223: 196: 176: 146: 97: 42: 1284:Meeten, G.H. (1986). 1170:Distinctness of image 981: 930: 889: 855: 828: 744: 721: 673: 650: 622: 606: 305: 244: 224: 222:{\displaystyle I_{r}} 197: 177: 175:{\displaystyle I_{0}} 147: 145:{\displaystyle R_{s}} 95: 40: 1014:reflected beam, B. 942: 902: 868: 840: 756: 733: 685: 659: 639: 316: 260: 233: 206: 186: 159: 129: 1335:Physical properties 976: 925: 884: 850: 823: 739: 716: 668: 645: 625: 601: 300: 239: 219: 192: 172: 142: 98: 68:surface topography 43: 1274:978-0-8031-7017-9 973: 820: 781: 648:{\displaystyle i} 615:Surface roughness 584: 581: 524: 448: 445: 398: 340: 298: 242:{\displaystyle m} 195:{\displaystyle i} 58:visual appearance 16:(Redirected from 1342: 1299: 1278: 1251: 1248: 1242: 1239: 1233: 1230: 1224: 1221: 1215: 1212: 1206: 1203: 1197: 1194: 1188: 1185: 1108: 1086: 1071: 1056: 1041: 1026: 985: 983: 982: 977: 974: 972: 955: 934: 932: 931: 926: 921: 893: 891: 890: 885: 859: 857: 856: 851: 832: 830: 829: 824: 821: 816: 793: 782: 777: 769: 748: 746: 745: 740: 725: 723: 722: 717: 677: 675: 674: 669: 654: 652: 651: 646: 610: 608: 607: 602: 600: 596: 595: 594: 589: 585: 583: 582: 574: 573: 561: 560: 551: 537: 536: 526: 525: 517: 516: 504: 503: 494: 480: 479: 469: 459: 458: 453: 449: 447: 446: 438: 437: 425: 424: 415: 400: 399: 391: 390: 378: 377: 368: 353: 341: 333: 328: 327: 309: 307: 306: 301: 299: 297: 296: 287: 286: 277: 272: 271: 254:Fresnel equation 248: 246: 245: 240: 228: 226: 225: 220: 218: 217: 201: 199: 198: 193: 181: 179: 178: 173: 171: 170: 151: 149: 148: 143: 141: 140: 41:Gloss reflection 21: 1350: 1349: 1345: 1344: 1343: 1341: 1340: 1339: 1320: 1319: 1306: 1296: 1283: 1275: 1262: 1259: 1254: 1249: 1245: 1240: 1236: 1231: 1227: 1222: 1218: 1213: 1209: 1204: 1200: 1195: 1191: 1186: 1182: 1178: 1161: 1136: 999: 959: 940: 939: 900: 899: 866: 865: 838: 837: 794: 770: 754: 753: 731: 730: 683: 682: 657: 656: 637: 636: 617: 565: 552: 528: 527: 508: 495: 471: 470: 464: 463: 429: 416: 401: 382: 369: 354: 348: 347: 346: 342: 319: 314: 313: 288: 278: 263: 258: 257: 231: 230: 209: 204: 203: 184: 183: 162: 157: 156: 132: 127: 126: 90: 35: 28: 23: 22: 15: 12: 11: 5: 1348: 1346: 1338: 1337: 1332: 1322: 1321: 1318: 1317: 1312: 1305: 1304:External links 1302: 1301: 1300: 1294: 1280: 1279: 1273: 1258: 1255: 1253: 1252: 1243: 1234: 1225: 1216: 1207: 1198: 1189: 1179: 1177: 1174: 1173: 1172: 1167: 1160: 1157: 1135: 1132: 1123: 1122: 1119: 1116: 1095: 1094: 1080: 1079: 1065: 1064: 1050: 1049: 1035: 1034: 1020: 1019: 1006:or "luster"). 998: 995: 987: 986: 971: 968: 965: 962: 958: 953: 950: 947: 924: 920: 916: 913: 910: 907: 882: 879: 876: 873: 848: 845: 834: 833: 819: 815: 812: 809: 806: 803: 800: 797: 791: 788: 785: 780: 776: 773: 767: 764: 761: 738: 727: 726: 714: 711: 708: 705: 702: 699: 696: 693: 690: 667: 664: 644: 629:surface finish 616: 613: 612: 611: 599: 593: 588: 580: 577: 572: 568: 564: 559: 555: 549: 546: 543: 540: 535: 531: 523: 520: 515: 511: 507: 502: 498: 492: 489: 486: 483: 478: 474: 467: 462: 457: 452: 444: 441: 436: 432: 428: 423: 419: 413: 410: 407: 404: 397: 394: 389: 385: 381: 376: 372: 366: 363: 360: 357: 351: 345: 339: 336: 331: 326: 322: 295: 291: 285: 281: 275: 270: 266: 238: 216: 212: 191: 169: 165: 139: 135: 115: 114: 111: 108: 105: 89: 86: 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 1347: 1336: 1333: 1331: 1328: 1327: 1325: 1316: 1313: 1311: 1308: 1307: 1303: 1297: 1295:0-85334-434-5 1291: 1287: 1282: 1281: 1276: 1270: 1267:. USA: ASTM. 1266: 1261: 1260: 1256: 1247: 1244: 1238: 1235: 1229: 1226: 1220: 1217: 1211: 1208: 1202: 1199: 1193: 1190: 1184: 1181: 1175: 1171: 1168: 1166: 1163: 1162: 1158: 1156: 1152: 1148: 1144: 1140: 1133: 1131: 1130:observation. 1128: 1120: 1117: 1114: 1113: 1112: 1109: 1107: 1102: 1098: 1092: 1091: 1090: 1087: 1085: 1077: 1076: 1075: 1072: 1070: 1062: 1061: 1060: 1057: 1055: 1047: 1046: 1045: 1042: 1040: 1032: 1031: 1030: 1027: 1025: 1017: 1016: 1015: 1011: 1007: 1003: 996: 994: 992: 969: 966: 963: 960: 956: 951: 948: 938: 937: 936: 922: 918: 914: 911: 908: 897: 880: 877: 874: 863: 846: 817: 813: 810: 807: 804: 798: 795: 789: 786: 778: 774: 771: 765: 762: 752: 751: 750: 736: 712: 709: 706: 703: 697: 694: 691: 681: 680: 679: 665: 642: 634: 630: 621: 614: 597: 591: 586: 578: 575: 570: 566: 562: 557: 553: 547: 544: 541: 538: 533: 529: 521: 518: 513: 509: 505: 500: 496: 490: 487: 484: 481: 476: 472: 465: 460: 455: 450: 442: 439: 434: 430: 426: 421: 417: 411: 408: 405: 402: 395: 392: 387: 383: 379: 374: 370: 364: 361: 358: 355: 349: 343: 337: 334: 329: 324: 320: 312: 311: 310: 293: 289: 283: 279: 273: 268: 264: 255: 250: 236: 214: 210: 189: 167: 163: 155: 137: 133: 123: 119: 112: 109: 106: 103: 102: 101: 94: 87: 85: 83: 81: 76: 71: 69: 65: 64: 59: 55: 51: 47: 39: 33: 19: 1285: 1264: 1246: 1237: 1228: 1219: 1210: 1201: 1192: 1183: 1153: 1149: 1145: 1141: 1137: 1124: 1110: 1103: 1099: 1096: 1088: 1081: 1073: 1066: 1058: 1051: 1043: 1036: 1028: 1021: 1012: 1008: 1004: 1000: 990: 988: 835: 728: 626: 251: 124: 120: 116: 99: 79: 74: 72: 61: 45: 44: 1324:Categories 1176:References 1127:glossmeter 633:micrometre 82:reflection 967:⁡ 957:λ 946:Δ 915:π 909:ϕ 906:Δ 881:π 875:ϕ 872:Δ 847:ϕ 844:Δ 818:λ 811:⁡ 802:Δ 799:π 784:Δ 779:λ 775:π 763:ϕ 760:Δ 737:λ 710:⁡ 701:Δ 689:Δ 663:Δ 576:⁡ 563:− 542:⁡ 519:⁡ 506:− 491:− 485:⁡ 440:⁡ 427:− 406:⁡ 393:⁡ 380:− 365:− 359:⁡ 154:intensity 1159:See also 75:specular 54:specular 1257:Sources 997:History 631:in the 80:diffuse 50:optical 32:Digiday 1330:Optics 1292:  1271:  88:Theory 48:is an 63:cesia 46:Gloss 1290:ISBN 1269:ISBN 952:< 912:< 252:The 964:cos 836:If 808:cos 707:cos 567:sin 539:cos 510:sin 482:cos 431:sin 403:cos 384:sin 356:cos 1326:: 993:. 249:. 70:. 1298:. 1277:. 970:i 961:8 949:h 923:2 919:/ 878:= 814:i 805:h 796:4 790:= 787:r 772:2 766:= 713:i 704:h 698:2 695:= 692:r 666:h 643:i 598:] 592:2 587:) 579:i 571:2 558:2 554:m 548:+ 545:i 534:2 530:m 522:i 514:2 501:2 497:m 488:i 477:2 473:m 466:( 461:+ 456:2 451:) 443:i 435:2 422:2 418:m 412:+ 409:i 396:i 388:2 375:2 371:m 362:i 350:( 344:[ 338:2 335:1 330:= 325:s 321:R 294:0 290:I 284:r 280:I 274:= 269:s 265:R 237:m 215:r 211:I 190:i 168:0 164:I 138:s 134:R 34:. 20:)

Index

Gloss (material appearance)
Digiday

optical
specular
visual appearance
cesia
surface topography
diffuse reflection

intensity
Fresnel equation

surface finish
micrometre
constructive interference
destructive interference
Specular gloss
Sheen
Contrast gloss
Absence of bloom
Distinctness of image gloss
Gloss-samples
glossmeter
List of optical topics
Distinctness of image
ISBN
978-0-8031-7017-9
ISBN
0-85334-434-5

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