ANALYZING EXISTING APPLIED MODELS OF THE IONOSPHERE FOR CALCULATING RADIO WAVE PROPAGATION AND POSSIBILITY OF THEIR USE FOR RADAR SYSTEMS. I. CLASSIFICATION OF APPLIED MODELS AND THE MAIN REQUIREMENTS IMPOSED ON THEM FOR RADAR AIDS

Journal Title: Solar-Terrestrial Physics - Year 2020, Vol 6, Issue 1

Abstract

We review modern HF–X band radars covering over-the-horizon problems. The ionosphere significantly affects wave propagation in all the bands. We describe available correction techniques, which use additional evidence on the ionosphere, as well as models of different degrees of complexity. The fact that the field of view cannot be covered by ground-based instruments as well as the growing requirements to the precision and stability of the radars result in the impossibility of ionospheric correction with up-to-date models, hence the latter require further elaboration. We give a virtually full classification of the models. The article summarizes the requirements to the models for the radars depending on their function.

Authors and Affiliations

Aksenov O. Yu. , Kozlov S. I. , Lyakhov A. N. , Trekin V. V. , Perunov Yu. M. , Yakubovsky S. V.

Keywords

Related Articles

INVESTIGATING THE INFLUENCE OF GEOMETRY OF THE HELIOSPHERIC NEUTRAL CURRENT SHEET AND SOLAR ACTIVITY ON MODULATION OF GALACTIC COSMIC RAYS WITH A METHOD OF MAIN COMPONENTS

The work studies the cumulative modulating effect of the geometry of the interplanetary magnetic field's neutral current sheet and solar activity on propagation of galactic cosmic rays in the heliosphere. The role of eac...

IDENTIFICATION OF SPECTRUM OF SECONDARY ACOUSTIC-GRAVITY WAVES IN THE MIDDLE AND UPPER ATMOSPHERE IN A HIGH-RESOLUTION NUMERICAL MODEL

Considerable attention has recently been paid to the study of so-called “secondary” acoustic-gravity waves (AGWs) that arise as a result of instability and nonlinear interactions of “primary” wave modes propagating from...

SECOND-ORDER PERTURBATIONS IN ALFVÉN WAVES IN COLD PLASMA APPROXIMATION

The second-order amplitude perturbations driven by Alfvén waves are studied. Equations for such second-order perturbations are derived and their solutions are found. The second-order perturbations are shown to be generat...

GEOMAGNETIC INDICES ASY-H AND SYM-H AND THEIR RELATION TO INTERPLANETARY PARAMETERS

The dependences of the geomagnetic indices SYM-H and ASY-H on interplanetary parameters for the period from 1981 to 2015 according to their daily averages are studied. The study is carried out in two ways: the first — th...

VARIATIONS OF FLOW DIRECTION IN SOLAR WIND STREAMS OF DIFFERENT TYPES

Studying the direction of the solar wind flow is a topical problem of space weather forecasting. As a rule, the quiet and uniform solar wind propagates radially, but significant changes in the solar wind flow direction c...

Download PDF file
  • EP ID EP700053
  • DOI 10.12737/stp-61202008
  • Views 87
  • Downloads 0

How To Cite

Aksenov O. Yu. , Kozlov S. I. , Lyakhov A. N. , Trekin V. V. , Perunov Yu. M. , Yakubovsky S. V. (2020). ANALYZING EXISTING APPLIED MODELS OF THE IONOSPHERE FOR CALCULATING RADIO WAVE PROPAGATION AND POSSIBILITY OF THEIR USE FOR RADAR SYSTEMS. I. CLASSIFICATION OF APPLIED MODELS AND THE MAIN REQUIREMENTS IMPOSED ON THEM FOR RADAR AIDS. Solar-Terrestrial Physics, 6(1), -. https://europub.co.uk/articles/-A-700053