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Staring array

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264:(VOx, pronounced "Vox"). A variety of lead salts can also be used, but are less common today. None of these materials can be grown into crystals anywhere near the size of modern silicon crystals, nor do the resulting wafers have nearly the uniformity of silicon. Furthermore, the materials used to construct arrays of IR-sensitive pixels cannot be used to construct the electronics needed to transport the resulting charge, voltage, or resistance of each pixel to the measurement circuitry. This set of functions is implemented on a chip called the 235:
similar fashion to a scanning array except that it images perpendicularly to the motion of the camera. A staring array is analogous to the film in a typical camera; it directly captures a 2-D image projected by the lens at the image plane. A scanning array is analogous to piecing together a 2D image with photos taken through a narrow slit. A TDI imager is analogous to looking through a vertical slit out the side window of a moving car, and building a long, continuous image as the car passes the landscape.
307:(PRNU). When un-illuminated, each pixel has a different "zero-signal" level, and when illuminated the delta in signal is also different. This non-uniformity makes the resulting images impractical for use until they have been processed to normalize the photo-response. This correction process requires a set of known characterization data, collected from the particular device under controlled conditions. The data correction can be done in software, in a 32: 238:
Scanning arrays were developed and used because of historical difficulties in fabricating 2-D arrays of sufficient size and quality for direct 2-D imaging. Modern FPAs are available with up to 2048 x 2048 pixels, and larger sizes are in development by multiple manufacturers. 320 x 256 and 640 x 480
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imagers in that they image the desired field of view without scanning. Scanning arrays are constructed from linear arrays (or very narrow 2-D arrays) that are rastered across the desired field of view using a rotating or oscillating mirror to construct a 2-D image over time. A TDI imager operates in
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in the visible spectrum. FPAs operate by detecting photons at particular wavelengths and then generating an electrical charge, voltage, or resistance in relation to the number of photons detected at each pixel. This charge, voltage, or resistance is then measured, digitized, and used to construct an
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A peculiar aspect of nearly all IR FPAs is that the electrical responses of the pixels on a given device tend to be non-uniform. In a perfect device every pixel would output the same electrical signal when given the same number of photons of appropriate wavelength. In practice nearly all FPAs have
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The difficulty in constructing high-quality, high-resolution FPAs derives from the materials used. Whereas visible imagers such as CCD and CMOS image sensors are fabricated from silicon, using mature and well-understood processes, IR sensors must be fabricated from other, more exotic materials
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or related weapons guidance sensors, infrared astronomy, manufacturing inspection, thermal imaging for firefighting, medical imaging, and infrared phenomenology (such as observing combustion, weapon impact, rocket motor ignition and other events that are interesting in the infrared spectrum).
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and between the FPA’s internal conductors. By replacing the receiver in the breadboard for one with a shorter focal length,  the focus of the collimator was reduced and the system’s threshold for signal recognition was increased. This facilitated a better image by cancelling cross talk.
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Itzler, Mark A.; Entwistle, Mark; Owens, Mark; Patel, Ketan; Jiang, Xudong; Slomkowski, Krystyna; Rangwala, Sabbir; Zalud, Peter F.; Senko, Tom (2010-08-19). Dereniak, Eustace L; Hartke, John P; Levan, Paul D; Sood, Ashok K; Longshore, Randolph E; Razeghi, Manijeh (eds.).
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Another method was to add a flat thinned substrate membrane (approximately 800 angstroms thick) to the FPA. This was reported to eliminate pixel-to-pixel cross talk in FPA imaging applications. In another an
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to collect and direct the breadboard’s laser beam onto individual pixels. Since low levels of voltage were still observed in pixels that did not illuminate, indicating that illumination was prevented by
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The low volumes, rarer materials, and complex processes involved in fabricating and using IR FPAs makes them far more expensive than visible imagers of comparable size and resolution.
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Marino, Richard M.; Stephens, Timothy; Hatch, Robert E; McLaughlin, Joseph L.; Mooney, James G.; O'Brien, Michael E.; Rowe, Gregory S.; Adams, Joseph S.; Skelly, Luke (2003-08-21).
187:. At optical and infrared wavelengths, it can refer to a variety of imaging device types, but in common usage it refers to two-dimensional devices that are sensitive in the 444:
Goldberg, A.; Stann, B.; Gupta, N. (July 2003). "Multispectral, Hyperspectral, and Three-Dimensional Imaging Research at the U.S. Army Research Laboratory" (PDF).
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D., Gunapala, S.; V., Bandara, S.; K., Liu, J.; J., Hill, C.; B., Rafol, S.; M., Mumolo, J.; T., Trinh, J.; Z., Tidrow, M.; D., LeVan, P. (May 2005).
562: 156:. FPAs are used most commonly for imaging purposes (e.g. taking pictures or video imagery), but can also be used for non-imaging purposes such as 248:
because silicon is sensitive only in the visible and near-IR spectra. Infrared-sensitive materials commonly used in IR detector arrays include
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Marino, Richard M.; Davis, William Rhett (2004). "Jigsaw : A Foliage-Penetrating 3 D Imaging Laser Radar System".
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or bonded to the ROIC, typically using indium bump-bonding, and the resulting assembly is called an FPA.
272:(ROIC), and is typically fabricated in silicon using standard CMOS processes. The detector array is then 269: 368: 231: 629: 288: 249: 578: 555: 308: 191:
spectrum. Devices sensitive in other spectra are usually referred to by other terms, such as CCD (
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arrays are available and affordable even for non-military, non-scientific applications.
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was reported with capabilities to repress cross talk between FPAs. Researchers at the
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FPA study, the etching of trenches in between neighboring pixels reduced cross talk.
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would swamp the detected signal. Devices can be cooled evaporatively, typically by
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in the camera electronics, or even on the ROIC in the most modern of devices.
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consisting of an array (typically rectangular) of light-sensing pixels at the
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temperatures, and others (such as resistive amorphous silicon (a-Si) and VOx
19:"Focal-plane array" redirects here. For arrays used in radio telescopes, see 157: 145: 265: 149: 389: 376: 602: 471: 381: 339: 280: 446:
Proceedings of the International Conference on International Fusion
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image of the object, scene, or phenomenon that emitted the photons.
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Detectors and Imaging Devices: Infrared, Focal Plane, Single Photon
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Some materials (and the FPAs fabricated from them) operate only at
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Focal plane arrays (FPAs) have been reported to be used for 3D
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both significant pixel-to-pixel offset and pixel-to-pixel
575: 56:. Unsourced material may be challenged and removed. 621: 211: 242: 464:Laser Radar Technology and Applications VIII 492: 561:CS1 maint: multiple names: authors list ( 116:Learn how and when to remove this message 16:Image sensor made of light-sensing pixels 532: 342:can inhibit the illumination of pixels. 321:Staring plane arrays are used in modern 203:Applications for infrared FPAs include 622: 295:(LN2) or liquid helium, or by using a 440: 438: 436: 429:Air-to-Air Weapons - Royal Air Force 384:. This cross talk was attributed to 260:(InGaAs, pronounced "Inn-Gas"), and 252:(HgCdTe, "MerCad", or "MerCadTel"), 54:adding citations to reliable sources 25: 411:Focal-plane array (radio astronomy) 350: 21:Focal-plane array (radio astronomy) 13: 14: 646: 466:. Vol. 5086. pp. 1–15. 433: 226:Staring arrays are distinct from 30: 362: 345: 256:(InSb, pronounced "Inns-Bee"), 41:needs additional citations for 569: 526: 486: 451: 422: 1: 462:. In Kamerman, Gary W (ed.). 416: 373:U.S. Army Research Laboratory 305:photo response non-uniformity 212:Comparison to scanning array 7: 404: 270:readout integrated circuits 10: 651: 243:Construction and materials 215: 18: 367:In 2003, a 32 x 32 pixel 250:mercury cadmium telluride 258:indium gallium arsenide 550:Cite journal requires 297:thermo-electric cooler 216:Further information: 193:charge-coupled device 399:avalanche photodiode 50:improve this article 595:2010SPIE.7780E..1MI 386:capacitive coupling 323:air-to-air missiles 222:Whisk broom scanner 134:staring-plane array 327:anti-tank missiles 218:Push broom scanner 166:wave-front sensing 603:10.1117/12.864465 514:Missing or empty 472:10.1117/12.501581 331:AIM-9X Sidewinder 262:vanadium(V) oxide 254:indium antimonide 197:CMOS image sensor 138:focal-plane array 126: 125: 118: 100: 642: 630:Infrared imaging 615: 614: 589:. SPIE: 77801M. 573: 567: 566: 559: 553: 548: 546: 538: 530: 524: 523: 517: 512: 510: 502: 490: 484: 483: 455: 449: 442: 431: 426: 390:microstrip lines 351:3D LIDAR Imaging 132:, also known as 121: 114: 110: 107: 101: 99: 58: 34: 26: 650: 649: 645: 644: 643: 641: 640: 639: 620: 619: 618: 574: 570: 560: 551: 549: 540: 539: 531: 527: 515: 513: 504: 503: 491: 487: 456: 452: 443: 434: 427: 423: 419: 407: 365: 353: 348: 293:liquid nitrogen 285:microbolometers 245: 224: 214: 185:radio telescope 173:radio astronomy 122: 111: 105: 102: 65:"Staring array" 59: 57: 47: 35: 24: 17: 12: 11: 5: 648: 638: 637: 632: 617: 616: 568: 552:|journal= 525: 485: 450: 432: 420: 418: 415: 414: 413: 406: 403: 364: 361: 352: 349: 347: 344: 244: 241: 228:scanning array 213: 210: 124: 123: 38: 36: 29: 15: 9: 6: 4: 3: 2: 647: 636: 635:Image sensors 633: 631: 628: 627: 625: 612: 608: 604: 600: 596: 592: 588: 584: 580: 572: 564: 557: 544: 536: 529: 521: 508: 500: 496: 489: 481: 477: 473: 469: 465: 461: 454: 448:. 1: 499–506. 447: 441: 439: 437: 430: 425: 421: 412: 409: 408: 402: 400: 394: 391: 387: 383: 378: 374: 370: 360: 358: 343: 341: 337: 336: 332: 328: 324: 319: 316: 314: 310: 306: 300: 298: 294: 290: 289:thermal noise 286: 282: 277: 275: 271: 267: 263: 259: 255: 251: 240: 236: 233: 229: 223: 219: 209: 206: 201: 198: 194: 190: 186: 182: 178: 174: 169: 167: 163: 159: 155: 151: 147: 143: 139: 135: 131: 130:staring array 120: 117: 109: 98: 95: 91: 88: 84: 81: 77: 74: 70: 67: –  66: 62: 61:Find sources: 55: 51: 45: 44: 39:This article 37: 33: 28: 27: 22: 586: 582: 571: 543:cite journal 528: 488: 463: 453: 445: 424: 395: 388:between the 366: 363:Improvements 354: 346:Applications 338: 329:such as the 320: 317: 301: 278: 273: 246: 237: 225: 202: 170: 158:spectrometry 146:image sensor 141: 137: 133: 129: 127: 112: 103: 93: 86: 79: 72: 60: 48:Please help 43:verification 40: 266:multiplexer 150:focal plane 106:August 2018 624:Categories 516:|url= 417:References 377:collimator 369:breadboard 340:Cross talk 274:hybridized 179:is at the 76:newspapers 611:120955542 480:110267445 382:crosstalk 359:imaging. 281:cryogenic 144:), is an 507:cite web 499:18046922 405:See also 189:infrared 591:Bibcode 375:used a 205:missile 90:scholar 609:  497:  478:  335:ASRAAM 195:) and 175:, the 164:, and 92:  85:  78:  71:  63:  607:S2CID 495:S2CID 476:S2CID 357:LIDAR 268:, or 183:of a 181:focus 162:LIDAR 152:of a 97:JSTOR 83:books 587:7780 563:link 556:help 520:help 325:and 313:FPGA 230:and 220:and 154:lens 69:news 599:doi 468:doi 311:or 309:DSP 232:TDI 177:FPA 171:In 142:FPA 136:or 52:by 626:: 605:. 597:. 585:. 581:. 547:: 545:}} 541:{{ 511:: 509:}} 505:{{ 474:. 435:^ 333:, 299:. 168:. 160:, 128:A 613:. 601:: 593:: 565:) 558:) 554:( 537:. 522:) 518:( 501:. 482:. 470:: 140:( 119:) 113:( 108:) 104:( 94:· 87:· 80:· 73:· 46:. 23:.

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Focal-plane array (radio astronomy)

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"Staring array"
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image sensor
focal plane
lens
spectrometry
LIDAR
wave-front sensing
radio astronomy
FPA
focus
radio telescope
infrared
charge-coupled device
CMOS image sensor
missile
Push broom scanner
Whisk broom scanner
scanning array
TDI

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