Microphysical characteristics of shallow precipitating systems in the southwest monsoon season: An analysis using in-situ and remote sensing observations
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引用次数: 0
Abstract
The present study examined the microphysical features of the shallow precipitating systems at low (10.04°N, 76.33°E, 20 m above MSL) and mid-altitude (8.45°N, 77.5°E; 400 m above MSL) locations situated on the windward side of the Western Ghats in southwest monsoon 2019. A total of 226 and 336 shallow precipitating systems were identified using radar reflectivity and surface rain rate from the co-located measurements using the micro rain radar and disdrometer instruments in both locations. The average cloud base height of shallow precipitating systems is ∼1 km. An elevated cloud layers (0.8–3.8 km) during long-duration shallow precipitating systems are more prevalent in low-altitude location. Shallow events in the mid-altitude region are characterized by long durations and high surface rain rates. Based on the duration and rain rates, the shallow systems are further classified for in-depth microphysical analysis. The broader raindrop size distribution spectra are clearly observed for the shallow events having higher duration and intensity. The concentration of small size raindrops are higher across all rain categories in the low-altitude location, while the concentration of mid-sized raindrops is notably higher in the heavy rain category indicating an active collision-coalescence process. Light rain events are predominantly characterized by small raindrops (D < 1 mm), whereas moderate and heavy rainfall events are primarily composed of midsize raindrops (1 ≤ D < 3 mm). The Nw-Dm relation for the shallow events in wet (dry) spells suggests that, isolated events mainly occur due to the local orographic effects of the elevated terrains.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.