K. Nishimura | Masashi Kohma

Latest

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
Estimate of Turbulent Energy Dissipation Rate From the VHF Radar and Radiosonde Observations 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
Turbulent kinetic energy dissipation rate derived from multi-year observations by radar and radiosonde in the Antarctic
Seasonal variation of energy dissipation rate derived from radar and radiosonde observations at Syowa Station 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)
Energy dissipation rate estimation based on observations by the PANSY radar in the Antarctic
Characteristics of mesosphere echoes over Antarctica obtained using PANSY and MF radars
Quasi-12h inertia-gravity waves in the lower mesosphere observed by the PANSY radar at Syowa Station (39.6°E, 69.0°S)
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)