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Effect of magnetic storms and substorms on GPS slips at high latitudes
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  • 作者:V. I. Zakharov ; Yu. V. Yasyukevich ; M. A. Titova
  • 刊名:Cosmic Research
  • 出版年:2016
  • 出版时间:January 2016
  • 年:2016
  • 卷:54
  • 期:1
  • 页码:20-30
  • 全文大小:2,103 KB
  • 参考文献:1.Yeh, K.C. and Liu, C.H., Radio wave scintillations in the ionosphere, Proc. IEEE, 1982, vol. 70, no. 4, pp. 24–64.
    2.Pi, X., Mannucci, A.J., Lindqwister, U.J., and Ho, C.M., Monitoring of global ionospheric irregularities using the worldwide GPS network, Geophys. Res. Lett., 1997, vol. 24, no. 18, pp. 2283–2286.CrossRef ADS
    3.Ledvina, B.M., Makela, J.J., and Kintner, P.M., First observations of intense GPS L1 amplitude scintillations at midlatitude, Geophys. Res. Lett., 2002, vol. 29, no. 14. doi 10.1029/2002GL014770
    4.Ma, G.T., Maruyama a super bubble detected by dense GPS network at east Asian longitudes, Geophys. Res. Lett., 2006, vol. 33, L21103.CrossRef ADS
    5.Demyanov, V.V., Yasyukevich, Yu.V., Ishin, A.B., and Astafyeva, E.I., Effects of ionosphere super-bubble on the GPS positioning performance depending on the orientation relative to geomagnetic field, GPS Solutions, 2012, vol. 16, no. 2, pp. 181–189. doi 10.1007/s10291-011-0217-9CrossRef
    6.Afraimovich, E.L., Demyanov, V.V., Gavrilyuk, N.S., et al., Malfunction of satellite navigation systems GPS and GLONASS caused by powerful radio emission of the Sun during solar flares on December 6 and 13, 2006, and October 28, 2003, Cosmic Res., 2009, vol. 47, no. 2, pp. 126–137.CrossRef ADS
    7.Klobuchar, J.A., Kunches, J.M., and Van Dierendonck, A.J., Eye on the ionosphere: Potential solar radio burst effects on GPS signal to noise, GPS Solutions, 1999, vol. 3, no. 2, pp. 69–71.CrossRef
    8.Skone, S. and de Jong, M., Limitations in GPS receiver tracking performance under ionospheric scintillation, Phys. Chem. Earth, 2001, vol. 26, nos. 6–8, pp. 613–621.CrossRef
    9.Skone, S. and de Jong, M., The impact of geomagnetic substorms on GPS receiver performance, Earth, Planets Space, 2000, vol. 52, pp. 1067–1071.CrossRef ADS
    10.Doherty, P.H., Delay, S.H., Valladares, C.E., and Klobuchar, J.A., Ionospheric scintillation effects in the equatorial and auroral regions, in Proceedings of the International Beacon Satellite Symposium, June 4–6, 2001, Boston, 2001, pp. 328–333.
    11.Afraimovich, E.L., Lesyuta, O.S., Ushakov, I.I., and Voyeikov, S.V., Geomagnetic storms and the occurrence of phase slips in the reception of GPS signals, Ann. Geophys., 2002, vol. 45, no. 1, pp. 55–71.
    12.Afraimovich, E.L., Demyanov, V.V., and Kondakova, T.N., Degradation of performance of the navigation GPS system in geomagnetically disturbed conditions, GPS Solutions, 2003, vol. 7, no. 2, pp. 109–119.CrossRef
    13.Afraimovich, E.L., Astafyeva, E.I., Demyanov, V.V., et al., A review of GPS/GLONASS studies of the ionospheric response to natural and anthropogenic processes and phenomena, J. Space Weather Space Clim., 2013, vol. 3, p. A27.CrossRef ADS
    14.Jakowski, N., Stankov, S.M., and Klaehn, D., Operational space weather service for GNSS precise positioning, Ann. Geophys., 2005, vol. 23, pp. 3071–3079.CrossRef ADS
    15.Jakowski, N., Mayer, C., Wilken, V., and Borries, C., Ionospheric storms at high and mid-latitudes monitored by ground and space based GPS techniques, in Proceedings of the International Beacon Satellite Symposium, Boston College, June 11–15, Boston, 2007, pp. 48–53.
    16.Basu, Su., Basu, S., Makela, J.J., et al., Large magnetic storm-induced nighttime ionospheric flows at midlatitudes and their impacts on GPS-based navigation systems, Geophys. Res. Lett., 2008, vol. 113, A00A06. doi 10.1029/2008JA013076CrossRef
    17.Rama Rao, P.V.S., Gopi Krishna, S., Vara Prasad, J., et al., Geomagnetic storm effects on GPS based navigation, Ann. Geophys., 2009, vol. 27, pp. 2101–2110.CrossRef ADS
    18.Bergeot, N., Bruyninx, C., Defraigne, P., et al., Impact of the Halloween 2003 ionospheric storms on kinematic GPS positioning in Europe, GPS Solutions, 2011, vol. 15, pp. 171–180. doi 10.1007/s10291-010-0181-9CrossRef
    19.Demyanov, V.V., Yasyukevich, Yu.V., and Jin, S., Effects of solar radio emission and ionospheric irregularities on GPS/GLONASS performance, in Geodetic Sciences—Observations, Modeling and Applications, Jin, S., Ed., InTech, 2013, pp. 177–222.
    20.Astafyeva, E., Yasyukevich, Y., Maksikov, A., and Zhivetiev, I., Geomagnetic storms, super-storms, and their impacts on GPS-based navigation systems, Space Weather, 2014, vol. 12, no. 7, pp. 508–525. doi 10.1002/2014SW001072CrossRef ADS
    21.Afraimovich, E.L., Dem’yanov, V.V., and Kondakova, T.N., Quality analysis of the operation of dualfrequency GPS receivers during geomagnetic storms, Issledovano v Rossi, 2004, no. 6, pp. 164–173. http://​zhurnal.​ape.​relarn.​ru/​articles/​2004/​016.​pdf
    22.Kaplan, E.D., Understanding GPS: Principles and Applications, Boston: Artech House, 1996.
    23.Aarons, J. and Lin, B.J., Development of high-latitude phase fluctuations during the January 10, April 10–11, and May 15, 1997 magnetic storms, J. Atmos. Sol.–Terr. Phys., 1999, vol. 61, pp. 309–327.CrossRef ADS
    24.Mushini, S.C., Jayachandran, P.T., Langley, R.B., and Pokhotelov, D., Improved amplitude- and phase-scintillation indices derived from wavelet detrended highlatitude GPS data, GPS Solutions, 2012, vol. 16, no. 3, pp. 363–373. doi 10.1007/s10291-011-0238-4CrossRef
    25.Basu, S., Basu, S., MacKenzie, E., and Whitney, H.E., Morphology of phase and intensity scintillations in the auroral oval and polar cap, Radio Sci., 1985, vol. 20, no. 3, pp. 347–356.CrossRef ADS
    26.Béniguel, Y., Forte, B., Radicella, S.M., et al., Scintillations effects on satellite to Earth links for telecommunication and navigation purposes, Ann. Geophys., 2004, vol. 47, nos. 2–3, pp. 1179–1199.
    27.Meggs, R.W., Mitchell, C.M., and Honary, F., GPS scintillation over the European Arctic during the November 2004 storms, GPS Solutions, 2008, vol. 12, pp. 281–287.CrossRef
    28.Kuznetsov, V.D., Space weather and risks of space activity, Kosm. Tekh. Tekhnol., 2014, no. 3, pp. 3–13.
    29.Hofmann-Wellenhof, B., Lichtenegger, H., and Collins, J., GPS: Theory and Practice, New York: Springer, 1998.
    30.Dow, J.M., Neilan, R.E., and Rizos, C., The international GNSS service in a changing landscape of global navigation satellite systems, J. Geod., 2009, vol. 83, nos. 3–4, pp. 191–198. doi 10.1007/s00190-008-0300-3CrossRef ADS
    31.Jayachandran, P.T., Langley, R.B., MacDougall, J.W., et al., The Canadian High Arctic Ionospheric Network (CHAIN), Radio Sci., 2009, no. 44, RS0A03. doi 10.1029/2008RS004046CrossRef
    32.Global Positioning Systems Directorate, Systems Engineering and Integration Interface Specification IS-GPS-200. September 5, 2012. http://​www.​gps.​gov/​technical/​icwg/​/​IS-GPS-200G.​pdf
  • 作者单位:V. I. Zakharov (1) (2)
    Yu. V. Yasyukevich (2)
    M. A. Titova (3)

    1. Faculty of Physics, Moscow State University, Moscow, 119991, Russia
    2. Institute of Solar–Terrestrial Physics, Siberian Division, Russian Academy of Sciences, ul. Lermontova 126a, Irkutsk, 664033, Russia
    3. Institute of Terrestrial Magnetism, the Ionosphere, and the Radio-Wave Propagation, Russian Academy of Sciences, Moscow, 142190, Russia
  • 刊物类别:Physics and Astronomy
  • 刊物主题:Physics
    Astronomy, Astrophysics and Cosmology
    Astrophysics
    Extraterrestrial Physics and Space Sciences
    Russian Library of Science
  • 出版者:MAIK Nauka/Interperiodica distributed exclusively by Springer Science+Business Media LLC.
  • ISSN:1608-3075
文摘
The dynamics of slips in navigation signal parameters of GPS from 2010 to 2014 is considered for the stations of the IGS and CHAIN networks located in the Arctic region. On the basis of almost continuous (more than 8 million hours) observations at around 200 receiving stations, we investigate the probability of “instrumental” loss of phase and pseudo-range as well as short-term variations in the high rate of change of the total electron content (TEC) in different geomagnetic conditions. Quantitative estimates for the impact of geomagnetic disturbances on the slips of these parameters are given. The slip probabilities for TEC are significantly (100–200 times) higher than those of purely instrumental slips and grow during geomagnetic storms and substorms. The growth of instrumental slips may be caused by the increased absorption that occurs during geomagnetic storms, among other reasons, and is an indicator of auroral intrusions of highenergy particles. Original Russian Text © V.I. Zakharov, Yu.V. Yasyukevich, M.A. Titova, 2016, published in Kosmicheskie Issledovaniya, 2016, Vol. 54, No. 1, pp. 23–33.

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