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Structures and backscattering characteristics of CUSAT 205 MHz Stratosphere-Troposphere Radar at Cochin (10.04 o N, 76.3 o E) -First results
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  • Siddarth Shankar Das,
  • Nabarun Poddar,
  • Veenus Venugopal,
  • S Abhilash,
  • V Rakesh
Siddarth Shankar Das
Space Physics Laboratory, Vikram Sarabhai Space Centre

Corresponding Author:[email protected]

Author Profile
Nabarun Poddar
Department of Physics, University of Kerala, Space Physics Laboratory, Vikram Sarabhai Space Centre
Veenus Venugopal
Department of Physics, University of Kerala, Space Physics Laboratory, Vikram Sarabhai Space Centre
S Abhilash
Advanced Centre for Atmospheric Radar Research, Cochin University of Science and Technology
V Rakesh
Advanced Centre for Atmospheric Radar Research, Cochin University of Science and Technology

Abstract

This paper presents the first ever observations on aspect-sensitive characteristics of 205 MHz Stratosphere-troposphere radar located at a tropical station Cochin (10.04°N, 76.3°E) using volume scanning. The most significant and new observation is that the signal-to-noise ratio in zenith and off-zenith beams are nearly equal in some height region, indicating the presence of isotropic turbulence. Signal strength decreases by 0.75 dB per degree from 0 to 10 degree off-zenith, 0.9 dB per degree from 10 to 20 degree off-zenith and 0.3 dB per degree beyond 20 degree offzenith. Different causative mechanisms are discussed on the basis of various estimated parameters associated with aspect sensitivity. Maximum aspect sensitivity is observed between 12 and 17 km, indicating the presence of dynamic instability arising due to strong wind shear and atmospheric stability. When both the square of wind shear and stability parameters are above 0.25 × 10 −3 s −2 , the scatterers become mostly isotropic. The study also shows a power difference in the symmetric beams as well as azimuth angle dependency. Analysis suggests that this asymmetry is due to the tilting of layers by the action of atmospheric gravity waves generated through Kelvin-Helmholtz-instability. The
18 Mar 2024Submitted to ESS Open Archive
25 Mar 2024Published in ESS Open Archive