Peer-reviewed articles 17,970 +



Title: CHARACTERISTICS OF Pc5 PULSATIONS ACTIVITY AT MID LATITUDES DURING DECEMBER 2019

CHARACTERISTICS OF Pc5 PULSATIONS ACTIVITY AT MID LATITUDES DURING DECEMBER 2019
Maria Chamati
10.5593/sgem2022/1.1
1314-2704
English
22
1.1
•    Prof. DSc. Oleksandr Trofymchuk, UKRAINE 
•    Prof. Dr. hab. oec. Baiba Rivza, LATVIA
Magnetospheric pulsations and the mechanisms underlying their generation are topics under active studies. The Pc5 (f =1.7–6.7 mHz) geomagnetic continuous pulsations, recorded at mid latitudes (L =1.6) during December 2019, with a low level of geomagnetic activity, are analyzed and discussed in this paper. The data sets of the series on geomagnetic field variations recorded at Panagjuriste Geomagnetic Observatory in Bulgaria are analyzed. The spectral characteristics of the pulsations were determined by Continuous Wavelet Analysis (CWT). It is demonstrated that Pc5 pulsation activity appears with all ranges of periods (140-600s) on December 6, 8, and 18, 2019, at time intervals of 02-17 UTC, 14-20 UTC, and 00-16 UTC, respectively. Then, the solar wind (SW) plasma speed, the flow dynamic pressure, and the geomagnetic index Kp are computed for every case of recorded Pc5 pulsations. It is suggested that recorded continuous pulsations in the Pc5 range are due to step-like or sudden increases in solar wind oscillations and variations of the flow dynamic pressure, which precede the appearance of pulsations and drive compressional magnetic field variations in the magnetosphere.
[1] McPherron RL. Magnetic Pulsations: Their Sources and Relationto Solar Wind and Geomagnetic Activity. Surv Geophys 2005;26:545–92. https://doi.org/10.1007/s10712- 005-1758-7.
[2] Hudson M, Denton R, Lessard M, Miftakhova E, Anderson R. A study of Pc-5 ULF oscillations. Annales Geophysicae 2004;22:289–302. https://doi.org/10.5194/angeo-22- 289-2004.
[3] Kwon H-J, Kim K-H, Jee G, Jin H, Kim H, Shin J, et al. Characteristics of Pc5 activity at high latitudes stations in Antarctica. Journal of Atmospheric and Solar-Terrestrial Physics 2019;193:105087. https://doi.org/10.1016/j.jastp.2019.105087.
[4] Oliva D, Meirelles MC, Papa ARR. A Study of Pc4-5 Geomagnetic Pulsations in the Brazilian Sector. ArXiv:14044321 [Physics] 2014.
[5] Liu W, Sarris TE, Li X, Elkington SR, Ergun R, Angelopoulos V, et al. Electric and magnetic field observations of Pc4 and Pc5 pulsations in the inner magnetosphere: A statistical study. Journal of Geophysical Research: Space Physics 2009;114. https://doi.org/10.1029/2009JA014243.
[6] Belakhovsky V, Pilipenko V, Murr D, Fedorov E, Kozlovsky A. Modulation of the ionosphere by Pc5 waves observed simultaneously by GPS/TEC and EISCAT. Earth, Planets and Space 2016;68:102. https://doi.org/10.1186/s40623-016-0480-7.
[7] Liu W, Sarris TE, Li X, Ergun R, Angelopoulos V, Bonnell J, et al. Solar wind influence on Pc4 and Pc5 ULF wave activity in the inner magnetosphere. Journal of Geophysical Research: Space Physics 2010;115. https://doi.org/10.1029/2010JA015299.
[8] El-Eraki MA, Rabeh T, Lethy A, Ghamry E, Samy A. Detection of long period Pc5 pulsation during 01st/Jul/2011 to 30th/Jun/2012 recorded at Egyptian and some INTERMAGNET observatories. NRIAG Journal of Astronomy and Geophysics 2014;3:192–7. https://doi.org/10.1016/j.nrjag.2014.11.001.
[9] Hynonen R, Tanskanen EI, Francia P. Solar cycle evolution of ULF wave power in solar wind and on ground. J Space Weather Space Clim 2020;10:43. https://doi.org/10.1051/swsc/2020046.
[10] Kepko L, Spence HE, Singer HJ. ULF waves in the solar wind as direct drivers of magnetospheric pulsations. Geophysical Research Letters 2002;29:39-1-39–4. https://doi.org/10.1029/2001GL014405.
[11] Kim K-H, Cattell CA, Lee D-H, Takahashi K, Yumoto K, Shiokawa K, et al. Magnetospheric responses to sudden and quasiperiodic solar wind variations. Journal of Geophysical Research: Space Physics 2002;107:SMP 36-1-SMP 36-12. https://doi.org/10.1029/2002JA009342.
This study was supported by the Contract No D01-404/18.12.2020 (Project "National Geoinformation Center (NGIC))", financed by the National Roadmap for Scientific Infrastructure 2020-2027 of Bulgaria.
M. Chamati would like to thank to Dr. M. Velante and Dr. E. Pietropaolo from University of L’Aquila, Italy to assistance. We thank the OMNIWEB database for data provided about IMF Bz, Kp index, SW speed, and flow dynamic pressure.
conference
Proceedings of 22nd International Multidisciplinary Scientific GeoConference SGEM 2022
22nd International Multidisciplinary Scientific GeoConference SGEM 2022, 04 - 10 July, 2022
Proceedings Paper
STEF92 Technology
International Multidisciplinary Scientific GeoConference SGEM
SWS Scholarly Society; Acad Sci Czech Republ; Latvian Acad Sci; Polish Acad Sci; Serbian Acad Sci and Arts; Natl Acad Sci Ukraine; Natl Acad Sci Armenia; Sci Council Japan; European Acad Sci, Arts and Letters; Acad Fine Arts Zagreb Croatia; Croatian Acad Sci and Arts; Acad Sci Moldova; Montenegrin Acad Sci and Arts; Georgian Acad Sci; Acad Fine Arts and Design Bratislava; Turkish Acad Sci.
509-516
04 - 10 July, 2022
website
8446
Pc5 pulsations, geomagnetic field, spectral characteristics