Abolfazl Neyestani
@razi.ac.ir
Department of physics
Razi University
EDUCATION
PhD in Meteorology
RESEARCH INTERESTS
Numerical weather prediction
Data assimilation
Forecast verification
Wavelet and spectral analysis
Climate variability
Scopus Publications
Scholar Citations
Scholar h-index
Scholar i10-index
Scopus Publications
Abolfazl Neyestani, Khalil Karami, and Siavash Gholami
Elsevier BV
Abolfazl Neyestani, Nils Gustafsson, Sarmad Ghader, Ali Reza Mohebalhojeh, and Heiner Körnich
Elsevier BV
K. Karami, S. Ghader, A. A. Bidokhti, M. Joghataei, A. Neyestani, and A. Mohammadabadi
American Geophysical Union (AGU)
[1] It is believed that in the lower ionosphere, particularly in the ionospheric sporadic E (Es) layers (90–130 km), the planetary and tidal wave-type oscillations in the ionized component indicate the planetary and tidal waves in the neutral atmosphere. In the present work, the presence of wave-type oscillations, including planetary and tidal waves in the ionospheric sporadic E layers over Tehran region is examined. Data measured by a digital ionosonde at the ionospheric station of the Institute of Geophysics, University of Tehran, from July 2006 to June 2007 are used to investigate seasonal variations of planetary and tidal waves activities. For the purpose of accurate comparison between different seasons, wavelet transform is applied to time series of foEs and h′Es, namely, the critical frequency and virtual height of Es layers, respectively. The results show that the sporadic E layers over Tehran region are strongly under the influence of upward propagation of waves from below. More specifically, among diverse range of periodicities in the sporadic E layers, we found that diurnal (24 hours) and semidiurnal (12 hours) oscillations in all seasons for both parameters. Moreover, terdiurnal (8 hours) tide-like variation is observed during spring and summer for foEs parameter and summer and winter for h′Es. Furthermore, the results show that diurnal tidal waves obtain their maximum activities during autumn and winter seasons, and their activities decrease during the late spring and summer. In addition, periods of about 2, 4, 6, 10, 14, and 16 days in our observation verifies the hypothesis of upward propagation of planetary waves from lower atmosphere to the ionosphere. Moreover, planetary waves have their maximum activities during equinox.