Periods of planetary waves, especially the 10- and 16-day waves, were found in Fourier analyses of 10-year geomagnetic time series from two mid-latitude stations in the northern hemisphere. This suggests that planetary waves influence geomagnetic variations. Cross-spectral analysis of magnetic time series from seven stations located at around 50°N at the beginning of 1979, when a 16-day wave occurred in the stratosphere, also shows a 16-day oscillation. However, study of the phases does not reveal the horizontal direction of wave propagation. Furthermore, the temporal variations of the 16-day oscillation in magnetic time series are presented as dynamic spectra and the results are compared with global investigations of geopotential ...
This paper summarizes the results of our research in sporadic E-layer (Es) dynamics with planetary w...
1. The period of the magnetic pulsations has no sharply defined value, varying from about 20 seconds...
Long-period oscillations in the period range 2–30 days, interpreted as planetary wave (PW) si...
Geomagnetic data from five northern hemisphere observatories at latitudes ranging from 22 degrees N ...
A network of 15 northern hemisphere radars has been used to measure horizontal winds in the mesosphe...
In an earlier study based upon medium frequency radar (MFR) data from Saskatoon (52°N) the variabili...
The spatial structure of the planetary waves in the frequency parameters of the sporadic E layer hav...
Zonal and meridional winds in the equatorial mesosphere and lower thermosphere (65-98 km) measured a...
The interannual variability of the seasonal evolution in the southern hemisphere is investigated, us...
The mesospheric and lower thermospheric (MLT) winds (60–100 km) obtained by multiple MF radars, lo...
New mechanisms for imposing planetary wave (PW) variability on the ionosphere‐thermosphere system ar...
This study examines the role of traveling planetary waves in producing day-to-day variability of the...
The ionosphere is mainly influenced by the sun through electromagnetic radiation and particle precip...
Complex studies with the use of spectrum and harmonic analysis allow determination of wave disturban...
Frequency spectra of magnetic pulsations of frequency range from 5 to 100 mHz observed at temperate ...
This paper summarizes the results of our research in sporadic E-layer (Es) dynamics with planetary w...
1. The period of the magnetic pulsations has no sharply defined value, varying from about 20 seconds...
Long-period oscillations in the period range 2–30 days, interpreted as planetary wave (PW) si...
Geomagnetic data from five northern hemisphere observatories at latitudes ranging from 22 degrees N ...
A network of 15 northern hemisphere radars has been used to measure horizontal winds in the mesosphe...
In an earlier study based upon medium frequency radar (MFR) data from Saskatoon (52°N) the variabili...
The spatial structure of the planetary waves in the frequency parameters of the sporadic E layer hav...
Zonal and meridional winds in the equatorial mesosphere and lower thermosphere (65-98 km) measured a...
The interannual variability of the seasonal evolution in the southern hemisphere is investigated, us...
The mesospheric and lower thermospheric (MLT) winds (60–100 km) obtained by multiple MF radars, lo...
New mechanisms for imposing planetary wave (PW) variability on the ionosphere‐thermosphere system ar...
This study examines the role of traveling planetary waves in producing day-to-day variability of the...
The ionosphere is mainly influenced by the sun through electromagnetic radiation and particle precip...
Complex studies with the use of spectrum and harmonic analysis allow determination of wave disturban...
Frequency spectra of magnetic pulsations of frequency range from 5 to 100 mHz observed at temperate ...
This paper summarizes the results of our research in sporadic E-layer (Es) dynamics with planetary w...
1. The period of the magnetic pulsations has no sharply defined value, varying from about 20 seconds...
Long-period oscillations in the period range 2–30 days, interpreted as planetary wave (PW) si...