Masashi Kohma
Masashi Kohma
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Estimation of turbulent energy dissipation rates by a VHF radar in the Antarctic
Weakening of PMWE and Turbulent Energy Dissipation Rates after a Stratospheric Sudden Warming in the Southern Hemisphere in 2019
Time variations of PMWE and turbulent energy dissipation rate after SSW in the Southern Hemisphere in 2019
A statistical analysis of the energy dissipation rate estimated from the PMWE spectral width in the Antarctic
A statistical analysis of the turbulent parameters of the PMWE observed by the PANSY radar at Syowa Station (69S, 40E) in the Antarctic
A statistical analysis of the spectral width of the PMWE observed by the PANSY radar at Syowa Station (69°S, 40°E) in the Antarctic
A statistical analysis of the spectral width of the PMWE observed by the PANSY radar at Syowa Station (69°S, 40°E) in the Antarctic
Turbulent Kinetic Energy Dissipation Rates Depending on the Polar Vortex and on Synoptic-scale Disturbances in the UTLS Region in the Antarctic
Simultaneous observations of polar mesosphere winter echoes and cosmic noise absorptions in a common volume by the PANSY radar (69.0°S, 39.6°E)
Quasi-12h inertia-gravity waves in the lower mesosphere observed by the PANSY radar at Syowa Station (39.6°E, 69.0°S)
Frequency spectra and vertical profiles of wind fluctuations in the summer Antarctic mesosphere revealed by MST radar observations
Characteristics of Vertical Wind Fluctuations in the Lower Troposphere at Syowa Station in the Antarctic Revealed by the PANSY Radar
Height and time characteristics of seasonal and diurnal variations in PMWE based on 1 year observations by the PANSY radar (69.0°S, 39.6°E)
Program of the Antarctic Syowa MST/IS radar (PANSY)
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