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Global Oscillations Network Group

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126: 64: 51: 318: 35: 153: 242:). With these sites, GONG typically can observe the Sun 91% of the time, 24/7. GONG was constructed to provide observations for helioseismology, which aims to understand the solar interior by analyzing the sound waves that are trapped in it. In 2001, the original GONG detectors were upgraded to 1000 x 1000 pixels and continuous 365:
Harvey, J. W.; Hill, F.; Hubbard, R. P.; Kennedy, J. R.; Leibacher, J. W.; Pintar, J. A.; Gilman, P. A.; Noyes, R. W.; Title, A. M.; Toomre, J.; Ulrich, R. K.; Bhatnagar, A.; Kennewell, J. A.; Marquette, W.; Patrón, J.; Saá, O.; Yasukawa, E. (31 May 1996). "The Global Oscillation Network Group (GONG)
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reported on the importance of GONG and its successor data source for space weather operations. It concluded that "GONG provides a vital data source for space weather operations, and it is nearing end of life. The ngGONG project is the most straightforward replacement. It will maintain present
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Pevtsov, Alexei A.; Martinez-Pillet, V.; Gilbert, H.; de Wijn, A. G.; Roth, M.; Gosain, S.; Upton, L. A.; Katsukawa, Y.; Burkepile, J.; Zhang, Jie; Reardon, K. P.; Bertello, L.; Jain, K.; Tripathy, S. C.; Leka, K. D. (2022-11-12). "Helio2024 Science White Paper: ngGONG -- Future Ground-based
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operational capabilities, and provide observations for future requirements. The time window to complete ngGONG prior to the demise of GONG is closing." The Board recommended that "NOAA/NWS financially support the design phase for ngGONG, to insure the initiation of the project."
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were implemented, and the new system is known as GONG++. While GONG still provides helioseismology data, it now also provides full-disk solar magnetic field maps (magnetograms) every minute and full-disk images of the Sun in the wavelength of the
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Deployed in 1995, GONG is a set of six observing systems geographically distributed around the Earth so that the Sun can be observed as continuously as possible. The six observatories are the
278: 156: 235: 183:. The network serves multiple purposes, including the provision of operation data for use in space weather prediction, and the study of solar 267: 255:
are used for research into the solar magnetic field and chromosphere but are also essential inputs into forecasts of space weather. The NOAA
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is proposing to design and build a next-generation Ground-based solar Observing Network, provisionally named ngGONG. In April 2023,
329: 256: 317: 305: 555: 282: 521: 252: 350: 286: 274: 211: 100: 522:"Statement on Global Oscillation Network Group (GONG) and its Successor Data Source for Space Weather Operations" 227: 219: 457: 403:"The Global Oscillation Network Group Facility—An Example of Research to Operations in Space Weather" 179:(GONG) is a worldwide network of six identical telescopes, designed to have 24/7 observations of the 125: 501: 481: 447: 260: 17: 473: 435: 383: 243: 207: 195: 119: 465: 414: 375: 436:"Continuous Solar Observations from the Ground—Assessing Duty Cycle from GONG Observations" 188: 461: 199: 63: 549: 485: 50: 434:
Jain, Kiran; Tripathy, Sushanta C.; Hill, Frank; Pevtsov, Alexei A. (2021-10-01).
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Facilities for Research in Heliophysics and Space Weather Operational Forecast".
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Spain, Australia, United States of America, India, Chile
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Integrated Synoptic Program (NISP), which is operated by
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Publications of the Astronomical Society of the Pacific
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NOAA Science Advisory Board Reports, Report Library
133: 115: 107: 96: 70: 57: 44: 335:GONG at Big Bear Solar Observatory, California 8: 27: 124: 62: 49: 26: 505: 451: 418: 357: 301: 281:under a cooperative agreement with the 236:Cerro Tololo Inter-American Observatory 28:Global Oscillation Network Group (GONG) 251:spectral line every 20 seconds. These 268:Community Coordinated Modeling Center 7: 311:GONG shelter in Learmonth, Australia 273:The GONG Project is managed by the 323:GONG shelter at Mauna Loa, Hawai'i 103:Integrated Synoptic Program (NISP) 25: 48:Global Oscillation Network Group 328: 316: 304: 177:Global Oscillation Network Group 151: 33: 18:Global Oscillation Network Group 257:Space Weather Prediction Center 1: 380:10.1126/science.272.5266.1284 401:Hill, Frank (October 2018). 291:NOAA Science Advisory Board 283:National Science Foundation 204:Learmonth Solar Observatory 572: 351:National Solar Observatory 275:National Solar Observatory 212:Big Bear Solar Observatory 101:National Solar Observatory 228:Udaipur Solar Observatory 162: 149: 32: 470:10.1088/1538-3873/ac24d5 259:(SWPC), the US Airforce 157:Related media on Commons 45:Alternative names 220:Mauna Loa Observatory 420:10.1029/2018SW002001 116:Telescope style 39:Map of GONG stations 556:Solar observatories 462:2021PASP..133j5001J 374:(5266): 1284–1286. 187:and dynamics using 29: 261:557th Weather Wing 185:internal structure 413:(10): 1488–1497. 208:Western Australia 196:Teide Observatory 173: 172: 120:solar observatory 16:(Redirected from 563: 541: 540: 538: 536: 526: 518: 512: 511: 509: 496: 490: 489: 455: 446:(1028): 105001. 431: 425: 424: 422: 398: 392: 391: 362: 332: 320: 308: 166:edit on Wikidata 155: 145: 142: 140: 129: 128: 92: 89: 87: 85: 83: 81: 79: 77: 66: 53: 37: 30: 21: 571: 570: 566: 565: 564: 562: 561: 560: 546: 545: 544: 534: 532: 531:. 27 April 2023 524: 520: 519: 515: 498: 497: 493: 433: 432: 428: 400: 399: 395: 364: 363: 359: 343: 336: 333: 324: 321: 312: 309: 300: 249:Hydrogen–α (Hα) 189:helioseismology 169: 137: 123: 74: 40: 23: 22: 15: 12: 11: 5: 569: 567: 559: 558: 548: 547: 543: 542: 513: 491: 426: 393: 356: 355: 354: 342: 341:External links 339: 338: 337: 334: 327: 325: 322: 315: 313: 310: 303: 299: 296: 200:Canary Islands 171: 170: 163: 160: 159: 147: 146: 135: 131: 130: 117: 113: 112: 109: 105: 104: 98: 94: 93: 72: 68: 67: 59: 55: 54: 46: 42: 41: 38: 24: 14: 13: 10: 9: 6: 4: 3: 2: 568: 557: 554: 553: 551: 530: 523: 517: 514: 508: 503: 495: 492: 487: 483: 479: 475: 471: 467: 463: 459: 454: 449: 445: 441: 437: 430: 427: 421: 416: 412: 408: 407:Space Weather 404: 397: 394: 389: 385: 381: 377: 373: 369: 361: 358: 352: 348: 345: 344: 340: 331: 326: 319: 314: 307: 302: 297: 295: 292: 288: 284: 280: 276: 271: 269: 266: 262: 258: 254: 253:data products 250: 245: 241: 237: 233: 229: 225: 221: 217: 213: 209: 205: 201: 197: 192: 190: 186: 182: 178: 167: 161: 158: 154: 148: 144: 136: 132: 127: 121: 118: 114: 110: 106: 102: 99: 95: 91: 73: 69: 65: 60: 56: 52: 47: 43: 36: 31: 19: 533:. Retrieved 528: 516: 494: 443: 439: 429: 410: 406: 396: 371: 367: 360: 298:GONG Gallery 272: 244:magnetograms 193: 176: 174: 97:Organization 71:Coordinates 58:Location(s) 507:2211.06712 453:2110.06319 366:Project". 279:AURA, Inc. 263:, and the 234:) and the 216:California 486:238362018 478:0004-6280 347:GONG info 550:Category 458:Bibcode 388:8662455 368:Science 349:at the 226:), the 218:), the 210:), the 202:), the 134:Website 535:12 May 484:  476:  386:  224:Hawaii 150:  122:  82:/sites 525:(PDF) 502:arXiv 482:S2CID 448:arXiv 240:Chile 232:India 164:[ 108:Built 90:.html 86:_long 537:2024 474:ISSN 384:PMID 353:site 265:NASA 175:The 143:.edu 141:.nso 139:gong 111:1995 88:_elv 84:/lat 80:.edu 78:.nso 76:gong 466:doi 444:133 415:doi 376:doi 372:272 287:NSO 181:Sun 552:: 527:. 480:. 472:. 464:. 456:. 442:. 438:. 411:16 409:. 405:. 382:. 370:. 191:. 539:. 510:. 504:: 488:. 468:: 460:: 450:: 423:. 417:: 390:. 378:: 238:( 230:( 222:( 214:( 206:( 198:( 168:] 20:)

Index

Global Oscillation Network Group
GONG network sites map
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gong.nso.edu/sites/lat_long_elv.html
National Solar Observatory
solar observatory
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gong.nso.edu

Related media on Commons
edit on Wikidata
Sun
internal structure
helioseismology
Teide Observatory
Canary Islands
Learmonth Solar Observatory
Western Australia
Big Bear Solar Observatory
California
Mauna Loa Observatory
Hawaii
Udaipur Solar Observatory
India
Cerro Tololo Inter-American Observatory
Chile
magnetograms
Hydrogen–α (Hα)
data products

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