Disturbances of GLONASS and GPS signals during magnetic storm on March 23—24, 2023, according to observations on the Kola peninsula

Capa

Citar

Texto integral

Acesso aberto Acesso aberto
Acesso é fechado Acesso está concedido
Acesso é fechado Somente assinantes

Resumo

The growth of scintillations of GLONASS and GPS satellite signals using the Septentrio GNSS receiver installed in the city of Apatity during a strong magnetic storm on March 23—24, 2023, is analyzed. According to the ionosonde data at the Lovozero station and the data of the EISCAT radar in Tromsø, it was shown that the growth of phase scintillations is caused by an increase in the plasma concentration mainly in the E-layer of the ionosphere. The growth of phase scintillations is accompanied by the appearance of discrete forms of auroras.

Texto integral

Acesso é fechado

Sobre autores

V. Belakhovsky

Polar Geophysical Institute

Autor responsável pela correspondência
Email: belakhov@mail.ru
Rússia, Apatity

A. Vasilev

Fedorov Institute of Applied Geophysics

Email: belakhov@mail.ru
Rússia, Moscow

A. Kalishin

Arctic and Antarctic Research Institute

Email: belakhov@mail.ru
Rússia, Saint Petersburg

A. Roldugin

Polar Geophysical Institute

Email: belakhov@mail.ru
Rússia, Apatity

Bibliografia

  1. Yeh K.C., Liu C.H. // Proc. IEEE. 1982. V. 70. No. 4. P. 24.
  2. Basu S., Groves K.M., Basu S., Sultan P.J. // J. Atm. Solar-Terr. Phys. 2002. V. 64. No. 16. P. 1745.
  3. Kintner P.M., Ledvina B.M., De Paula E.R. // Space Weather. 2007. V. 5. Art. No. S0900.
  4. Astafyeva E., Yasyukevich Yu., Maksikov A., Zhivetiev I. // Space Weather. 2014. V. 12. No. 7. P. 508.
  5. Черноус С.А., Шагимуратов И.И., Иевенко И.Б. и др. // Хим. физика. 2018. Т. 37. № 5. С. 77; Chernous S.A., Shagimuratov I.I., Ievenko I.B. et al. // Russ. J. Phys. Chem. 2018. V. 12. No. 3. P. 562.
  6. Черноус С.А., Швец М.В., Филатов М.В. и др. // Хим. физика. 2015. Т. 34. № 10. С. 33; Chernous S.A., Shvets M.V., Filatov M.V. et al. // Russ. J. Phys. Chem. 2015. V. 9. No. 5. P. 778.
  7. Шагимуратов И.И., Филатов М.В., Ефишов И.И. и др. // Изв. РАН. Сер. физ. 2021. Т. 85. № 3. С. 433; Shagimuratov I.I., Filatov M.V., Efishov I.I. et al. // Bull. Russ. Acad. Sci. Phys. 2021. V. 85. No. 3. P. 318.
  8. Smith A.M., Mitchell C.N., Watson R.J. et al. // Space Weather. 2008. V. 6. Art. No. s03d01.
  9. Prikryl P., Jayachandran P.T., Mushini S.C. et al. // Ann. Geophys. 2010. V. 28. P. 1307.
  10. Makarevich R.A., Crowley G., Azeem I. et al. // J. Geophys. Res. 2021. V. 126. Art. No. e2021JA029212.
  11. Belakhovsky V.B., Jin Y., Miloch W.J. // Ann. Geophys. 2021. V. 39. P. 687.
  12. Белаховский В.Б., Джин Я., Милош В. // Совр. пробл. дист. зонд. Земли из косм. 2020. Т. 17. № 6. С. 139.
  13. Белаховский В.Б., Джин Я., Милош В. // Изв. РАН. Сер. физ. 2022. Т. 86. № 3. С. 428; Belakhovsky V.B., Jin Y., Miloch W. // Bull. Russ. Acad. Sci. Phys. 2022. V. 86. No. 3. P. 348.
  14. Ясюкевич Ю.В., Живетьев И.В., Ясюкевич А.С. и др. // Совр. пробл. дист. зонд. Земли из косм. 2017. Т. 14. № 1. С. 88.
  15. Захаров В.И., Ясюкевич Ю.В., Титова М.А. // Косм. иссл. 2016. Т. 54. № 1. С. 23; Zakharov V.I., Yasyukevich Yu.V., Titova M.A. // Cosmic Res. 2016. V. 54. No. 1. P. 20.
  16. Chernyshov A.A., Miloch W.J., Jin Y., Zakharov V.I. // Sci. Reports. 2020. V. 10. Art. No. 6363.
  17. Russell C.T., McPherron R.L. // J. Geophys. Res. 1973. V. 78. P. 92.
  18. Mushini S.C., Jayachandran P.T., Langley R.B. et al. // GPS Solutions. 2012. V. 16. P. 363.
  19. Forte B. // J. Atm. Sol.-Terr. Phys. 2005. V. 67. P. 1100.
  20. Lyatsky W., Elphinstone R.D., Pao Q., Cogger L.L. // J. Geophys. Res. 1999. V. 104. No. A1. P. 263.
  21. Белаховский В.Б., Пилипенко В.А., Самсонов С.Н., Лоренцен Д. // Геомагн. и аэроном. 2016. Т. 56. № 1. С. 46; Belakhovsky V.B., Pilipenko V.A., Samsonov S.N., Lorentsen D. // Geomagn. Aeronomy. 2016. V. 56. No. 1. P. 42.
  22. Van der Meeren C., Oksavik K., Lorentzen D. et al. // J. Geophys. Res. 2014. V. 119. P. 8624.
  23. Miller K.L., Smith L.G. // J. Geophys. Res. 1978. V. 83. No. A8. P. 3761.
  24. Miyoshi Y., Oyama S., Saito S. et al. // J. Geophys. Res. 2015. V. 120. P. 2754.

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML
2. Fig. 1. Variations of solar wind velocity V, solar wind density N, MMP modulus B, Bz-component of MMP, AE-index, SYM-H-index for 23-24 March 2023

Baixar (724KB)
3. Fig. 2. Phase (σF), amplitude (S4) indices of scintillations at the L1 frequency from the data of the receiver at the APT station (Apatity) for GPS and GLONASS satellites; variations of X-, Y-components of the geomagnetic field from the data of the Lovozero Observatory, variations of X-, Y-components of the geomagnetic field with the removed low-frequency trend (0.5 mHz) from the data of the Lovozero Observatory for 23-24 March 2023

Baixar (911KB)
4. Fig. 3. Variations of ionospheric plasma concentration from EISCAT UHF radar data in Tromsø with height; variations of ionospheric plasma concentration at heights of 110, 152, 282 km; phase index of scintillations for GLONASS satellites from the data of the receiver at the APT station (Apatity)

Baixar (1MB)
5. Fig. 4. Daily variations of critical frequencies of the ionosphere on 23-24 March 2023, ionograms from the ionosonde data at HMS Lovozero station at 12.39 UT, 20.24 UT - 23.03.2023, at 18.09 UT, 19.09 UT - 24.03.2023

Baixar (1MB)
6. Fig. 5. Frames of the all-sky camera at Lovozero Observatory on 23 March 2023 for the time moments 18.46, 19.15, 20.27 UT (upper panel), 20.37, 21.27, 23.45 UT (lower panel)

Baixar (402KB)

Declaração de direitos autorais © Russian Academy of Sciences, 2024