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Bolometer

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bolometer, and remarked that it was a beautiful instrument. I then said, "Professor Langley, I have a suggestion for making an improvement in the bolometer, if you will embody it in the principle." I explained to him how the bolometer could be improved. Professor Langley was very much interested and wrote in his notebook what I suggested. I used what I have termed a small-mass resistance, but of much smaller mass than in the bolometer of Langley, and of much smaller mass than that of any of the devices which have been recorded in patents issued since. Those are clumsy things. I used masses that were not a millionth of the smallest mass described in any of the patents, or in the publications. With such an instrument, I operated, for instance, in West Point—I received signals from my laboratory on Houston Street in West Point.
343:(ECRH). In terms of hardware, the W7-X bolometers are equipped with metal-resistive detectors. These are distinguished by a 5 μm thick gold absorber, sized 1.3 mm in the poloidal direction and 3.8 mm toroidally, mounted on a ceramic (silicon nitride Si3N4) substrate. The inclusion of a 50 nm carbon layer is strategic, enhancing the detection efficiency for low-energy photons. These detectors are notably attuned to impurity line radiation, covering a spectrum from the very ultraviolet (VUV) to soft x-rays (SXR). Given their resilience and innovative design, they are being considered as prototypes for the upcoming 62: 22: 396:. This resistance change is measured and processed into temperatures which can be represented graphically. The microbolometer grid is commonly found in three sizes, a 640×480 array, a 320×240 array (384×288 amorphous silicon) or less expensive 160×120 array. 640x512 VOx arrays are commonly used in static security camera applications with low shock resistance requirements. Different arrays provide the same resolution with larger array providing a wider 160:); this lack of discrimination can also be a shortcoming. The most sensitive bolometers are very slow to reset (i.e., return to thermal equilibrium with the environment). On the other hand, compared to more conventional particle detectors, they are extremely efficient in energy resolution and in sensitivity. They are also known as thermal detectors. 120:
A bolometer consists of an absorptive element, such as a thin layer of metal, connected to a thermal reservoir (a body of constant temperature) through a thermal link. The result is that any radiation impinging on the absorptive element raises its temperature above that of the reservoir – the greater
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employs a two-camera bolometer system to capture plasma radiation. This setup is optimized to identify 2D radiation distributions within a symmetrical triangular plasma cross-section. Recent progress includes the refinement of a tomographic reconstruction algorithm, which leans on the principle of
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to the waveguide characteristic impedance. After applying microwave power, the bias current is reduced to return the bolometer to its resistance in the absence of microwave power. The change in the dc power is then equal to the absorbed microwave power. To reject the effect of ambient temperature
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I suppose I had hundreds of devices, but the first device that I used, and it was very successful, was an improvement on the bolometer. I met Professor Langley in 1892 at the Royal Institution. He said to me, after I had delivered a lecture, that they were all proud of me. I spoke to him of the
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and connected to a battery. Electromagnetic radiation falling on the exposed strip would heat it and change its resistance. By 1880, Langley's bolometer was refined enough to detect thermal radiation from a cow a quarter of a mile (400 m) away. This radiant-heat detector is sensitive to
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system. Power coupled to the electron system drives it out of thermal equilibrium with the phonon system, creating hot electrons. Phonons in the metal are typically well-coupled to substrate phonons and act as a thermal reservoir. In describing the performance of the HEB, the relevant
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materials at low temperature. If the absorbing element does not have a temperature-dependent resistance, as is typical of normal (non-superconducting) metals at very low temperature, then an attached resistive thermometer can be used to measure the electron temperature.
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with an identical element not exposed to microwaves; variations in temperature common to both elements do not affect the accuracy of the reading. The average response time of the bolometer allows convenient measurement of the power of a pulsed source.
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personally asked Dr. Langley whether he could use his bolometer for his power transmission experiments in 1892. Thanks to that first use, he succeeded in making the first demonstration between West Point and his laboratory on Houston Street.
318:). Their use as particle detectors was proposed from the beginning of the 20th century, but the first regular, though pioneering, use was only in the 1980s because of the difficulty associated with cooling and operating a system at 133:, or the resistance of the absorptive element itself can be used as a thermometer. Metal bolometers usually work without cooling. They are produced from thin foils or metal films. Today, most bolometers use 193:
differences in temperature of one hundred-thousandth of a degree Celsius (0.00001 °C). This instrument enabled him to thermally detect across a broad spectrum, noting all the chief
298:. They use the same principle described above. The bolometers are sensitive not only to light but to every form of energy. The operating principle is similar to that of a 543: 722:
NIKOLA TESLA ON HIS WORK WITH ALTERNATING CURRENTS and Their Application to Wireless Telegraphy, Telephony and Transmission of Power : An Extended Interview
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of the absorbing element depends on the electron temperature, then the resistance can be used as a thermometer of the electron system. This is the case for both
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frequencies. In this application, a resistive element is exposed to microwave power. A dc bias current is applied to the resistor to raise its temperature via
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the absorbed power, the higher the temperature. The intrinsic thermal time constant, which sets the speed of the detector, is equal to the ratio of the
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Bolometers are directly sensitive to the energy left inside the absorber. For this reason they can be used not only for ionizing particles and
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In 2020, two groups reported microwave bolometers based on graphene-based materials capable of microwave detection at the single-photon level.
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of high energy physics, these devices are not called "calorimeters", since this term is already used for a different type of detector (see
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relative gradient smoothing (RGS) of emission profiles. This has been effectively applied to the W7-X hydrogen discharges powered by
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between the absorptive element and the reservoir. The temperature change can be measured directly with an attached resistive
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at these wavelengths. To achieve the best sensitivity, they must be cooled to a fraction of a degree above
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Wellstood, F. C.; Urbina, C.; Clarke, John (1994). "Hot-electron effects in metals".
892: 831: 754: 725: 677: 471: 374: 370: 295: 185: 1048: 1164: 1078: 1009: 1001: 923: 878: 843: 821: 813: 652: 604: 291: 246:). Notable examples of bolometers employed in submillimeter astronomy include the 685: 331: 194: 61: 197:. He also discovered new atomic and molecular absorption lines in the invisible 883: 858: 445: 366: 362: 356: 303: 138: 1082: 1005: 688:). High Altitude Observatory, University Corporation for Atmospheric Research. 330:
Bolometers play a pivotal role in monitoring radiation in fusion plasmas. The
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While bolometers can be used to measure radiation of any frequency, for most
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and is measured with a resistive thermometer, allowing the determination of
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The structure and function of a pit organ has similarities to a bolometer.
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ranges there are other methods of detection that are more sensitive. For
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absorptive elements rather than metals. These devices can be operated at
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Langley, S. P. (12 January 1881). "The Bolometer and Radiant Energy".
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bolometers – Definition from the Merriam-Webster Online Dictionary
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strikes the vanadium oxide or amorphous silicon, and changes its
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Lee, Gil-Ho; Efetov, Dmitri K.; et al. (1 October 2020).
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Kokkoniemi, R.; Girard, J.-P.; et al. (1 October 2020).
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temperatures, enabling significantly greater sensitivity.
1118:"New microwave bolometers could boost quantum computers" 645:
Proceedings of the American Academy of Arts and Sciences
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is a specific type of bolometer used as a detector in a
972:"Graphene-based Josephson junction microwave bolometer" 16:
Device for measuring incident electromagnetic radiation
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The first bolometers made by Langley consisted of two
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by means of a material having a temperature-dependent
905: 49:. It was invented in 1878 by the American astronomer 969: 285: 152:, but also for non-ionizing particles, any sort of 400:. Larger, 1024×768 arrays were announced in 2008. 429:is the electronic heat capacity and the relevant 325: 1156: 1150:Langley's own words on the bolometer and its use 775:"CMB-S4 – CMB-S4 Next Generation CMB Experiment" 470:changes, the active (measuring) element is in a 412:temperatures, typically within a few degrees of 256:Stratospheric Observatory for Infrared Astronomy 1141:(Richards group, Dept. of Physics, UC Berkeley) 642: 621: 585:"Bolometers for infrared and millimeter waves" 408:The hot electron bolometer (HEB) operates at 108:. The intrinsic thermal time constant is τ = 950:Encyclopedia of RF and Microwave Engineering 856: 791: 457:A bolometer can be used to measure power at 433:is the electron-phonon thermal conductance. 209: 25:Spiderweb bolometer for measurements of the 420:system in a metal is weakly coupled to the 578: 576: 377:heat sensors atop a corresponding grid of 1064: 987: 882: 825: 628:. American Metrological Society. p.  403: 201:portion of the electromagnetic spectrum. 56: 1115: 582: 452: 60: 20: 636: 615: 573: 242:(typically from 50 mK to 300  1157: 416:. At these very low temperatures, the 163: 748: 715: 27:cosmic microwave background radiation 1145:NASA on the history of the bolometer 1124:from the original on 8 October 2020. 1105:from the original on 5 October 2020. 1036:from the original on 5 October 2020. 751:Detectors and Sources for THz and IR 341:electron cyclotron resonance heating 1116:Johnston, Hamish (5 October 2020). 622:Langley, S. P. (23 December 1880). 290:The term bolometer is also used in 66:Conceptual schematic of a bolometer 13: 350: 188:which was fitted with a sensitive 14: 1196: 1132: 125:of the absorptive element to the 798:Review of Scientific Instruments 544:"Langley's Bolometer, 1880-1890" 286:Applications in particle physics 1109: 1040: 963: 942: 899: 857:Zhang, D.; et al. (2021). 850: 792:Zhang, D.; et al. (2010). 785: 767: 306:. However, the approximations, 294:to designate an unconventional 92:. The temperature increase is Δ 827:11858/00-001M-0000-0026-F070-5 749:Sizov, Fedir F. (5 May 2020). 742: 709: 691: 671: 561: 536: 465:, such that the resistance is 326:Applications in plasma physics 1: 529: 252:James Clerk Maxwell Telescope 7: 678:Samuel P. Langley Biography 481: 10: 1201: 1139:Introduction to bolometers 589:Journal of Applied Physics 523:Infrared sensing in snakes 354: 270:and the HFI camera on the 248:Herschel Space Observatory 220:sub-millimeter wavelengths 41:is a device for measuring 1185:Superconducting detectors 1083:10.1038/s41586-020-2753-3 1006:10.1038/s41586-020-2752-4 703:earthobservatory.nasa.gov 699:"Samuel Pierpont Langley" 388:from a specific range of 278:, CMB-S4 experiment, and 274:, as well as the planned 210:Applications in astronomy 180:foil strips covered with 928:10.1103/PhysRevB.49.5942 884:10.1088/1741-4326/ac2778 583:Richards, P. L. (1994). 493:Scintillating bolometer 51:Samuel Pierpont Langley 724:. Leland I. Anderson. 716:Tesla, Nikola (1992). 404:Hot electron bolometer 224:millimeter wavelengths 117: 57:Principle of operation 34: 1175:Measuring instruments 453:Microwave measurement 394:electrical resistance 347:bolometer detectors. 320:cryogenic temperature 308:ultra low temperature 64: 47:electrical resistance 24: 548:Science Museum Group 1075:2020Natur.586...47K 998:2020Natur.586...42L 920:1994PhRvB..49.5942W 875:2021NucFu..61k6043Z 810:2010RScI...81jE134Z 601:1994JAP....76....1R 431:thermal conductance 164:Langley's bolometer 127:thermal conductance 86:thermal conductance 80:, and temperature, 1180:Particle detectors 684:2009-11-06 at the 567:See, for example, 369:. It is a grid of 276:Simons Observatory 118: 35: 908:Physical Review B 818:10.1063/1.3483194 731:978-1-893817-01-2 375:amorphous silicon 296:particle detector 186:Wheatstone bridge 1192: 1126: 1125: 1113: 1107: 1106: 1068: 1044: 1038: 1037: 991: 967: 961: 948:Kai Chang (ed), 946: 940: 939: 914:(9): 5942–5955. 903: 897: 896: 886: 854: 848: 847: 829: 789: 783: 782: 771: 765: 764: 746: 740: 739: 713: 707: 706: 695: 689: 675: 669: 668: 657:10.2307/25138616 640: 634: 633: 619: 613: 612: 609:10.1063/1.357128 580: 571: 565: 559: 558: 556: 554: 540: 292:particle physics 272:Planck satellite 195:Fraunhofer lines 31:NASA/JPL-Caltech 29:. Image credit: 1200: 1199: 1195: 1194: 1193: 1191: 1190: 1189: 1155: 1154: 1135: 1130: 1129: 1114: 1110: 1059:(7827): 47–51. 1045: 1041: 982:(7827): 42–46. 968: 964: 960:pages 2736–2739 952:, (Wiley 2005) 947: 943: 904: 900: 855: 851: 790: 786: 773: 772: 768: 761: 747: 743: 732: 714: 710: 697: 696: 692: 686:Wayback Machine 676: 672: 641: 637: 625:The "Bolometer" 620: 616: 581: 574: 566: 562: 552: 550: 542: 541: 537: 532: 484: 455: 446:superconducting 406: 359: 353: 351:Microbolometers 332:Wendelstein 7-X 328: 288: 212: 166: 59: 17: 12: 11: 5: 1198: 1188: 1187: 1182: 1177: 1172: 1167: 1153: 1152: 1147: 1142: 1134: 1133:External links 1131: 1128: 1127: 1108: 1039: 962: 941: 898: 869:(11): 116043. 863:Nuclear Fusion 849: 804:(10): 10E134. 784: 766: 759: 741: 730: 708: 690: 670: 635: 614: 572: 560: 534: 533: 531: 528: 527: 526: 520: 515: 510: 505: 500: 495: 490: 483: 480: 472:bridge circuit 454: 451: 442:semiconducting 405: 402: 371:vanadium oxide 367:thermal camera 363:microbolometer 357:Microbolometer 355:Main article: 352: 349: 327: 324: 304:thermodynamics 287: 284: 211: 208: 165: 162: 139:superconductor 58: 55: 15: 9: 6: 4: 3: 2: 1197: 1186: 1183: 1181: 1178: 1176: 1173: 1171: 1168: 1166: 1163: 1162: 1160: 1151: 1148: 1146: 1143: 1140: 1137: 1136: 1123: 1119: 1112: 1104: 1100: 1096: 1092: 1088: 1084: 1080: 1076: 1072: 1067: 1062: 1058: 1054: 1050: 1043: 1035: 1031: 1027: 1023: 1019: 1015: 1014:1721.1/129674 1011: 1007: 1003: 999: 995: 990: 985: 981: 977: 973: 966: 959: 958:0-471-27053-9 955: 951: 945: 937: 933: 929: 925: 921: 917: 913: 909: 902: 894: 890: 885: 880: 876: 872: 868: 864: 860: 853: 845: 841: 837: 833: 828: 823: 819: 815: 811: 807: 803: 799: 795: 788: 780: 776: 770: 762: 760:9781644900741 756: 752: 745: 738: 733: 727: 723: 719: 712: 705:. 3 May 2000. 704: 700: 694: 687: 683: 679: 674: 666: 662: 658: 654: 650: 646: 639: 631: 627: 626: 618: 610: 606: 602: 598: 594: 590: 586: 579: 577: 570: 564: 549: 545: 539: 535: 524: 521: 519: 518:Pyrheliometer 516: 514: 511: 509: 506: 504: 501: 499: 496: 494: 491: 489: 486: 485: 479: 476: 473: 468: 464: 463:Joule heating 460: 450: 447: 443: 439: 434: 432: 428: 427:heat capacity 423: 419: 415: 414:absolute zero 411: 401: 399: 398:field of view 395: 391: 387: 384: 380: 376: 372: 368: 364: 358: 348: 346: 342: 337: 333: 323: 321: 317: 313: 309: 305: 301: 297: 293: 283: 281: 277: 273: 269: 265: 261: 257: 253: 249: 245: 241: 240:absolute zero 237: 233: 229: 225: 221: 217: 207: 204: 200: 196: 191: 187: 183: 179: 175: 171: 161: 159: 155: 151: 146: 144: 140: 136: 135:semiconductor 132: 128: 124: 123:heat capacity 115: 111: 107: 103: 99: 95: 91: 87: 83: 79: 75: 74:heat capacity 71: 67: 63: 54: 52: 48: 44: 40: 32: 28: 23: 19: 1111: 1056: 1052: 1042: 979: 975: 965: 949: 944: 911: 907: 901: 866: 862: 852: 801: 797: 787: 778: 769: 750: 744: 735: 721: 711: 702: 693: 673: 648: 644: 638: 624: 617: 592: 588: 563: 551:. Retrieved 547: 538: 488:Thermocouple 477: 456: 435: 407: 360: 329: 289: 213: 203:Nikola Tesla 190:galvanometer 167: 147: 119: 113: 109: 105: 101: 97: 93: 89: 81: 77: 69: 65: 43:radiant heat 38: 36: 18: 718:"section 4" 595:(1): 1–24. 390:wavelengths 336:stellarator 316:Calorimeter 300:calorimeter 282:satellite. 264:BICEP array 158:dark matter 131:thermometer 1170:Radiometry 1159:Categories 1066:2008.04628 989:1909.05413 779:cmb-s4.org 530:References 513:Thermistor 503:Radiometer 438:resistance 254:, and the 216:wavelength 1099:221095927 1030:202565642 893:238641528 508:Tasimeter 498:Pyrometer 459:microwave 410:cryogenic 386:radiation 236:astronomy 232:terahertz 182:lampblack 178:palladium 154:radiation 143:cryogenic 68:. Power, 39:bolometer 1122:Archived 1103:Archived 1091:32999484 1034:Archived 1022:32999482 936:10011570 836:21033996 682:Archived 665:25138616 553:20 March 482:See also 418:electron 383:Infrared 280:LiteBIRD 228:infrared 222:through 199:infrared 174:platinum 1165:Sensors 1071:Bibcode 994:Bibcode 916:Bibcode 871:Bibcode 844:3856215 806:Bibcode 651:: 348. 597:Bibcode 467:matched 436:If the 379:silicon 334:(W7-X) 150:photons 1097:  1089:  1053:Nature 1028:  1020:  976:Nature 956:  934:  891:  842:  834:  757:  728:  663:  422:phonon 312:jargon 268:SPT-3G 260:AdvACT 250:, the 1095:S2CID 1061:arXiv 1026:S2CID 984:arXiv 889:S2CID 840:S2CID 661:JSTOR 176:, or 170:steel 1087:PMID 1018:PMID 954:ISBN 932:PMID 832:PMID 755:ISBN 726:ISBN 555:2022 444:and 345:ITER 1079:doi 1057:586 1010:hdl 1002:doi 980:586 924:doi 879:doi 822:hdl 814:doi 653:doi 632:–7. 605:doi 373:or 302:in 137:or 1161:: 1120:. 1101:. 1093:. 1085:. 1077:. 1069:. 1055:. 1051:. 1032:. 1024:. 1016:. 1008:. 1000:. 992:. 978:. 974:. 930:. 922:. 912:49 910:. 887:. 877:. 867:61 865:. 861:. 838:. 830:. 820:. 812:. 802:81 800:. 796:. 777:. 734:. 720:. 701:. 659:. 649:16 647:. 603:. 593:76 591:. 587:. 575:^ 546:. 381:. 361:A 266:, 262:, 244:mK 230:, 172:, 96:= 88:, 76:, 53:. 37:A 1081:: 1073:: 1063:: 1012:: 1004:: 996:: 986:: 938:. 926:: 918:: 895:. 881:: 873:: 846:. 824:: 816:: 808:: 781:. 763:. 680:( 667:. 655:: 630:1 611:. 607:: 599:: 557:. 116:. 114:G 112:/ 110:C 106:P 102:G 100:/ 98:P 94:T 90:G 82:T 78:C 70:P 33:.

Index

Image of spiderweb bolometer for measurements of the cosmic microwave background radiation.
cosmic microwave background radiation
NASA/JPL-Caltech
radiant heat
electrical resistance
Samuel Pierpont Langley
Conceptual schematic of a bolometer.
heat capacity
thermal conductance
heat capacity
thermal conductance
thermometer
semiconductor
superconductor
cryogenic
photons
radiation
dark matter
steel
platinum
palladium
lampblack
Wheatstone bridge
galvanometer
Fraunhofer lines
infrared
Nikola Tesla
wavelength
sub-millimeter wavelengths
millimeter wavelengths

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