We analyse the lower ionosphere disturbances in the time period around the Mw 5.4 Kraljevo earthquake (EQ), which occurred on 3 November 2010 in Serbia. The results presented herein are based on analysis of the amplitudes of three VLF signals emitted in Italy, UK, and Germany and recorded in Serbia whose variations primarily result from changes in the electrical properties of the lower ionosphere at a distance more than 120 km from the epicentre of the EQ. The primary goals of this study are to reveal specific variations as possible EQ precursors as well as disturbances following the EQ event recorded by the observational equipment, and to investigate whether better time resolution data can affect the analysis of the lower ionosphere disturbances possibly connected to the EQ. We process two sets of data with sampling periods of 1 min and 0.1 s. As the first analysis indicates the absence of long-term disturbances, which can clearly be connected to the Kraljevo EQ, our attention is focused on the study of short-period noise amplitude and the excitation and attenuation of acoustic and gravity waves in the lower ionosphere. Processing of the amplitudes of three VLF signals during the nights of the four EQs with magnitude greater than 4 that occurred in Serbia, as well as EQs of all magnitudes during the three days of 3, 4, and 9 November, indicates that the detected ICV radio signal noise amplitude reduction starting before the Kaljevo EQ is also observed for 13 additional EQ events near the signal propagation path, and occurred during all three days (for all EQs with magnitude greater than 4 and several less intensive events). Excitation and attenuation of acoustic waves are also found for all these EQ events with a magnitude greater than 4.
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http://dx.doi.org/10.1016/j.scitotenv.2019.136406 | DOI Listing |
Heliyon
December 2024
Laser and Plasma Research Institute, Shahid Beheshti University, Tehran, 1983969411, Iran.
In this article, the propagation of high-frequency (HF) plane electromagnetic waves through the lower ionosphere is numerically investigated using the real geometry of the Earth's magnetic field in the northern hemisphere. For this purpose, the profiles of electron density and the collision frequency in the layers of the lower ionosphere (D- and E-region) are considered using the reported experimental data for day and night. The reflection, transmission, and absorption coefficients of HF radio waves in the frequency range of 3 to 30 MHz are calculated in the ionosphere plasma.
View Article and Find Full Text PDFSimultaneous observations of and in Jupiter's northern infrared aurora were conducted on 02 June 2017 using Keck-NIRSPEC to produce polar projection maps of radiance, rotational temperature, column density, and radiance. The temperature variations within the auroral region are K, generally consistent with previous studies, albeit with some structural differences. Known auroral heating sources including particle precipitation, Joule heating, and ion drag have been examined by studying the correlations between each derived quantity, yet no single dominant mechanism can be identified as the main driver for the energetics in Jupiter's northern auroral region.
View Article and Find Full Text PDFSci Rep
September 2024
Institute of Radio Physics and Electronics, University of Calcutta, Kolkata, West Bengal, India.
A VHF phased array radar for atmospheric dynamics observation is installed at the University of Calcutta, Kolkata. The Calcutta University Stratosphere-Troposphere Radar (CUSTR) operates at 53 MHz with 475 three sub-element Yagi-Uda antenna array. The CUSTR system is a high-power fully active phased array system with a dedicated 2 kW solid-state Transmit-Receiver Module (TRM) attached to each antenna, providing a total peak power of 950 kW with 47.
View Article and Find Full Text PDFJ Chem Phys
September 2024
Department of Physics, Utah State University, Logan, Utah 84322-4415, USA.
Experimental rate coefficients for the quenching of vibrational levels 0 and 1 of the N2+A2Πu state by N2 are presented. The experiments were performed using near-infrared observations of the N2+ Meinel bands excited by electron impact at several pressures of the N2 target/quenching gas. The total removal rate coefficients were derived from a Stern-Volmer analysis of the Meinel band intensities as a function of N2 density and yielded rate coefficients of (2.
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