Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Method of the HF wave absorption evaluation based on GIRO network data. / Zaalov, N. Y.; Moskaleva, E. V.; Shekhovtsov, F. V.
в: Advances in Space Research, Том 63, № 7, 01.04.2019, стр. 2075-2087.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Method of the HF wave absorption evaluation based on GIRO network data
AU - Zaalov, N. Y.
AU - Moskaleva, E. V.
AU - Shekhovtsov, F. V.
PY - 2019/4/1
Y1 - 2019/4/1
N2 - High frequency (HF) communication is strongly dependent on the state of the ionosphere, which specifies the mode structure of the radio wave propagating in ionosphere. Another core factor defining the strength of the HF signal at the receiving site is the ionospheric absorption. Accurate modelling the effect of absorption is an essential part of many studies of the HF propagation in the ionosphere. This paper proposes a method for estimating the absorption. The method is based on analysis of vertical sounding ionograms. The main idea of the approach is to compare the main parameters retrieved from measured and simulated ionograms. The combination of Global Ionospheric Radio Observatory (GIRO, http://giro.uml.edu) data and ionograms modelling allows for developing the empiric absorption model available at near real-time. The ionogram simulation taking into account absorption utilizes the NIM-RT (North Ionospheric Model and Ray Tracing) software. As a result, the proposed technique provides more reliable and accurate evaluation of minimum frequency at which echoes are observed in vertical incidence ionosonde soundings. The values of these frequencies should be used in the following simulation to optimize parameters in the empirical formulae for defining absorption HF wave in ionosphere. The ultimate objective of this work is the designing the method, which allows the simulating of HF radio channel accounting for regular absorption due to UV radiation of the Sun. Eventually it could be considered as some kind of the HF propagation forecasting.
AB - High frequency (HF) communication is strongly dependent on the state of the ionosphere, which specifies the mode structure of the radio wave propagating in ionosphere. Another core factor defining the strength of the HF signal at the receiving site is the ionospheric absorption. Accurate modelling the effect of absorption is an essential part of many studies of the HF propagation in the ionosphere. This paper proposes a method for estimating the absorption. The method is based on analysis of vertical sounding ionograms. The main idea of the approach is to compare the main parameters retrieved from measured and simulated ionograms. The combination of Global Ionospheric Radio Observatory (GIRO, http://giro.uml.edu) data and ionograms modelling allows for developing the empiric absorption model available at near real-time. The ionogram simulation taking into account absorption utilizes the NIM-RT (North Ionospheric Model and Ray Tracing) software. As a result, the proposed technique provides more reliable and accurate evaluation of minimum frequency at which echoes are observed in vertical incidence ionosonde soundings. The values of these frequencies should be used in the following simulation to optimize parameters in the empirical formulae for defining absorption HF wave in ionosphere. The ultimate objective of this work is the designing the method, which allows the simulating of HF radio channel accounting for regular absorption due to UV radiation of the Sun. Eventually it could be considered as some kind of the HF propagation forecasting.
KW - GIRO network
KW - HF wave propagation
KW - Ionogram processing
KW - Ionogram simulations
KW - NIM-RT software
KW - UV absorption
KW - OPTIMIZATION
KW - MODEL
KW - PROPAGATION
UR - http://www.scopus.com/inward/record.url?scp=85061052076&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2018.12.024
DO - 10.1016/j.asr.2018.12.024
M3 - Article
AN - SCOPUS:85061052076
VL - 63
SP - 2075
EP - 2087
JO - Advances in Space Research
JF - Advances in Space Research
SN - 0273-1177
IS - 7
ER -
ID: 39330282