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Heliospheric imager

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Heliospheric imagers are generally flown in space because the Earth's atmosphere itself interferes with the signal even at night. Terrestrial features such as clouds, aircraft, moonlight, small variations in dust and moisture content of the air column, and even high altitude
154:. Heliospheric imagers are simple in principle โ€“ they are simple visible light cameras placed inside deep optical baffles. However, the solar wind features are extremely faint โ€“ as little as 0.1% of the brightness of the background starfield and 178:
spacecraft in deep space. The concept was first demonstrated in the 1980s via detailed post-processing of photometer data from the two HELIOS spacecraft flown in the 1970s.
86: 170:, can obscure the desired solar wind signal. Instruments flown to date include the Solar Mass Ejection Imager (SMEI) flown on a 58: 65: 39: 315: 174:
satellite in high polar orbit, and the HI imagers that formed part of the SECCHI instrument suite on board NASA's twin
105: 72: 158: โ€“ and therefore heliospheric imager data require extensive post-processing to remove these backgrounds. 54: 43: 273: 79: 32: 339: 334: 308: 289: 243: 204: 8: 216: 247: 208: 344: 147: 301: 251: 212: 135: 285: 155: 256: 231: 328: 151: 123: 232:"Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)" 143: 21: 163: 175: 167: 146:. The electrons, in particular, scatter incident sunlight via 195:
Eyles, C. J. (2003). "The Solar Mass Ejection Imager (Smei)".
171: 150:, and clouds of plasma can therefore be photographed using 281: 139: 122:
is a wide-field camera that is designed to image the
126:in interplanetary space, far from the Sun itself. 46:. Unsourced material may be challenged and removed. 326: 309: 316: 302: 255: 106:Learn how and when to remove this message 327: 229: 194: 268: 44:adding citations to reliable sources 15: 13: 217:10.1023/B:SOLA.0000006903.75671.49 14: 356: 272: 20: 31:needs additional citations for 223: 188: 134:The solar wind is composed of 1: 181: 288:. You can help Knowledge by 280:This article related to the 7: 129: 10: 361: 267: 257:10.1007/s11214-008-9341-4 230:Howard, R. A. (2008). 236:Space Science Reviews 55:"Heliospheric imager" 40:improve this article 248:2008SSRv..136...67H 209:2003SoPh..217..319E 120:heliospheric imager 148:Thomson scattering 138:and contains both 297: 296: 116: 115: 108: 90: 352: 318: 311: 304: 276: 269: 262: 261: 259: 227: 221: 220: 192: 111: 104: 100: 97: 91: 89: 48: 24: 16: 360: 359: 355: 354: 353: 351: 350: 349: 325: 324: 323: 322: 266: 265: 228: 224: 193: 189: 184: 132: 112: 101: 95: 92: 49: 47: 37: 25: 12: 11: 5: 358: 348: 347: 342: 337: 321: 320: 313: 306: 298: 295: 294: 277: 264: 263: 222: 186: 185: 183: 180: 156:zodiacal light 131: 128: 114: 113: 28: 26: 19: 9: 6: 4: 3: 2: 357: 346: 343: 341: 340:Space imagers 338: 336: 335:Space weather 333: 332: 330: 319: 314: 312: 307: 305: 300: 299: 293: 291: 287: 283: 278: 275: 271: 270: 258: 253: 249: 245: 241: 237: 233: 226: 218: 214: 210: 206: 202: 198: 197:Solar Physics 191: 187: 179: 177: 173: 169: 165: 159: 157: 153: 152:visible light 149: 145: 141: 137: 127: 125: 121: 110: 107: 99: 88: 85: 81: 78: 74: 71: 67: 64: 60: 57: โ€“  56: 52: 51:Find sources: 45: 41: 35: 34: 29:This article 27: 23: 18: 17: 290:expanding it 279: 239: 235: 225: 203:(Nov): 319. 200: 196: 190: 160: 133: 119: 117: 102: 93: 83: 76: 69: 62: 50: 38:Please help 33:verification 30: 242:(1โ€“4): 67. 329:Categories 182:References 124:solar wind 66:newspapers 345:Sun stubs 144:electrons 142:and free 96:June 2017 130:Overview 244:Bibcode 205:Bibcode 164:airglow 80:scholar 176:STEREO 168:aurora 136:plasma 82:  75:  68:  61:  53:  284:is a 87:JSTOR 73:books 286:stub 172:USAF 166:and 140:ions 59:news 282:Sun 252:doi 240:136 213:doi 201:217 42:by 331:: 250:. 238:. 234:. 211:. 199:. 118:A 317:e 310:t 303:v 292:. 260:. 254:: 246:: 219:. 215:: 207:: 109:) 103:( 98:) 94:( 84:ยท 77:ยท 70:ยท 63:ยท 36:.

Index


verification
improve this article
adding citations to reliable sources
"Heliospheric imager"
news
newspapers
books
scholar
JSTOR
Learn how and when to remove this message
solar wind
plasma
ions
electrons
Thomson scattering
visible light
zodiacal light
airglow
aurora
USAF
STEREO
Bibcode
2003SoPh..217..319E
doi
10.1023/B:SOLA.0000006903.75671.49
"Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI)"
Bibcode
2008SSRv..136...67H
doi

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