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Argon flash

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168:, especially for photographing explosions, or less commonly for use in high altitude test vehicles. The photography of explosions and shock waves is made easy by the fact that the detonation of the argon flash lamp charge can be accurately timed relative to the test specimen explosion and the light intensity can overpower the light generated by the explosion itself. The formation of shock waves during explosions of 156:
as the explosion itself, depending on the construction of the lamp, between 0.1 and 100 microseconds. The duration is dependent on the length of the shockwave path through the gas, which is proportional to the length of the tube; it was shown that each centimeter of the path of shock wave through the argon medium is equivalent to 2 microseconds.
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The amount of explosive can control the intensity of the shock wave and therefore of the flash. The intensity of the flash can be increased and its duration decreased by reflecting the shock wave by a suitable obstacle; a foil or a curved glass can be used. The duration of the flash is about as long
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of the gas has to be compressed to sufficient temperature. The light intensity rises to full magnitude in about 0.1 microsecond. For about 0.5 microsecond the shock wave front instabilities are sufficient to create significant striations in the produced light; this effect diminishes as the thickness
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of the compressed layer increases. Only an about 75 micrometer thick layer of the gas is responsible for the light emission. The shock wave reflects after reaching the window at the end of the tube; this yields a brief increase of light intensity. The intensity then fades.
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charge. The explosion generates a shock wave, which heats the gas to very high temperature (over 10 K; published values vary between 15,000 K to 30,000 K with the best values around 25,000 K). The gas becomes
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Typical argon flash devices consist of an argon-filled cardboard or plastic tube with a transparent window on one end and an explosive charge on the other end. Many explosives can be used;
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Super Radiant Light (SRL) sources are an alternative to argon flash. An electron beam source delivers a brief and intense pulse of electrons to suitable crystals (e.g. doped
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is produced primarily by compression heating of the surrounding air. Replacement of the air with a noble gas considerably increases the light output; with
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is fairly high, significant heating of the illuminated object can occur. Especially in the case of high explosives, this has to be taken into account.
144:. The emission for the temperature range is highest between 97–193 nm, but usually only the visible and near-ultraviolet ranges are exploited. 252: 312: 282: 402: 302: 272: 397: 224: 122: 82: 407: 165: 94: 38:, is a single-use source of very short and extremely bright flashes of light. The light is generated by a 227:, William C. Davis, Terry R. Salyer, Scott I. Jackson, and Tariq D. Aslam, Los Alamos National Laboratory 141: 392: 304:
High-pressure shock compression of solids VIII: the science and technology of high-velocity impact
54:. Argon flash devices are almost exclusively used for photographing explosions and shock waves. 244: 364: 308: 278: 248: 354: 199: 183: 387: 176: 238: 381: 169: 148: 110: 134: 328: 97:
of noble gases allows heating to higher temperatures, yielding brighter emission.
138: 90: 86: 39: 186:). Flash times in the nanosecond to picosecond range are achievable. Pulsed 129: 98: 78: 74: 51: 47: 85:
and other processes, while noble gases are monatomic and can only undergo
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Single-use source of very short and extremely bright flash of light
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The device consists of a vessel filled with argon and a solid
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can be also used, argon is favored because of its low cost.
351:"Technical Report: High-Explosive Argon Flash Light Source" 301:
Lalit C. Chhabildas; Lee Davison; Yasuyuki Horie (2005).
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To achieve emission, the layer of at least one or two
237:Rudolf Meyer; Josef Köhler; Axel Homburg (2007). 101:are filled with noble gases for the same reason. 8: 81:gases, the energy is consumed partially by 50:. The shock wave is usually produced by an 274:Scientific photography and applied imaging 358: 137:and emits a flash of intense visible and 220: 218: 216: 214: 164:Argon flash is a standard procedure for 210: 349:Todd Jr, J; Parsons, D (1957-01-11). 225:Explosive-driven shock waves in argon 7: 296: 294: 14: 93:then produces the light. The low 1: 277:. Focal Press. p. 445. 46:or, less commonly, another 424: 331:. Yarchive.net. 1999-01-29 329:"Argon flash (Arno Hahma)" 175:As the amount of released 73:The light generated by an 307:. Springer. p. 263. 190:are another alternative. 125:are just a few examples. 123:plastic bonded explosives 172:can be imaged this way. 271:Sidney F. Ray (1999). 166:high-speed photography 95:specific heat capacity 403:Photographic lighting 243:. Wiley-VCH. p.  142:black-body radiation 36:argon light source 398:Flash photography 254:978-3-527-31656-4 415: 373: 372: 362: 346: 340: 339: 337: 336: 325: 319: 318: 298: 289: 288: 268: 262: 261: 234: 228: 222: 200:Sonoluminescence 28:argon flash bomb 22:, also known as 423: 422: 418: 417: 416: 414: 413: 412: 378: 377: 376: 360:10.2172/4310914 348: 347: 343: 334: 332: 327: 326: 322: 315: 300: 299: 292: 285: 270: 269: 265: 255: 236: 235: 231: 223: 212: 208: 196: 184:cadmium sulfide 162: 107: 71: 17: 12: 11: 5: 421: 419: 411: 410: 405: 400: 395: 390: 380: 379: 375: 374: 341: 320: 313: 290: 283: 263: 253: 229: 209: 207: 204: 203: 202: 195: 192: 177:radiant energy 170:shaped charges 161: 158: 149:optical depths 106: 103: 70: 67: 15: 13: 10: 9: 6: 4: 3: 2: 420: 409: 408:Types of lamp 406: 404: 401: 399: 396: 394: 391: 389: 386: 385: 383: 370: 366: 361: 356: 352: 345: 342: 330: 324: 321: 316: 314:3-540-22866-7 310: 306: 305: 297: 295: 291: 286: 284:0-240-51323-1 280: 276: 275: 267: 264: 260: 256: 250: 246: 242: 241: 233: 230: 226: 221: 219: 217: 215: 211: 205: 201: 198: 197: 193: 191: 189: 185: 180: 178: 173: 171: 167: 159: 157: 153: 150: 145: 143: 140: 136: 131: 126: 124: 120: 116: 112: 111:Composition B 104: 102: 100: 96: 92: 88: 84: 80: 76: 68: 66: 64: 60: 55: 53: 49: 45: 41: 37: 33: 29: 25: 21: 353:. Osti.gov. 344: 333:. Retrieved 323: 303: 273: 266: 259:Argon flash. 258: 239: 232: 181: 174: 163: 154: 146: 135:incandescent 127: 108: 83:dissociation 72: 56: 35: 32:argon candle 31: 27: 23: 19: 18: 139:ultraviolet 105:Engineering 91:ionized gas 20:Argon flash 393:Explosives 382:Categories 335:2010-03-23 240:Explosives 206:References 99:Flashtubes 87:ionization 40:shock wave 24:argon bomb 130:explosive 79:molecular 75:explosion 57:Although 52:explosion 48:noble gas 194:See also 369:4310914 69:Process 59:krypton 367:  311:  281:  251:  188:lasers 121:, and 89:; the 34:, and 388:Argon 63:xenon 44:argon 365:OSTI 309:ISBN 279:ISBN 249:ISBN 160:Uses 115:PETN 61:and 355:doi 119:RDX 42:in 384:: 363:. 293:^ 257:. 247:. 245:21 213:^ 117:, 113:, 30:, 26:, 371:. 357:: 338:. 317:. 287:.

Index

shock wave
argon
noble gas
explosion
krypton
xenon
explosion
molecular
dissociation
ionization
ionized gas
specific heat capacity
Flashtubes
Composition B
PETN
RDX
plastic bonded explosives
explosive
incandescent
ultraviolet
black-body radiation
optical depths
high-speed photography
shaped charges
radiant energy
cadmium sulfide
lasers
Sonoluminescence

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