Kaustav Chakravarty , Rohit P. Patil , Gargi Rakshit , G. Pandithurai
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引用次数: 0
Abstract
The paper aims to highlight the contrasting inter-seasonal variability of raindrop size distribution (DSD) as observed over Mumbai (representing a coastal city) and Mahabaleshwar (representing an orographic station in the Western Ghat mountain range) of Indian peninsula for a continuous period of four years (2018–2022). Upon examining the microphysical features of precipitation patterns, it is observed that raindrops with diameter of 3 mm and above dominate the rainfall in Mahabaleshwar during the pre-monsoon period, while the same with diameter of 1.5 mm and above dominate Mumbai's rainfall during the monsoon months. Additionally, the study finds a strong diurnal variation in rainfall occurrences during the pre-monsoon period for both the stations, while such variation is absent during the monsoon period. The analysis suggests that the Convective Available Potential Energy (CAPE) plays a significant role in these divergent diurnal patterns. Furthermore, the paper explores the relationship between mass-weighted mean diameter (Dm) - rain rate (R) values and shape (μ) versus slope (Λ) parameters as obtained from the two stations during the inter-seasonal phases of the monsoon. The results indicate that, during the pre-monsoon period, higher rain intensities (>16 mm/h) correspond to a dominant Dm value in Mahabaleshwar's rainfall. Conversely, during the monsoon months, higher Dm values are noticeable in Mumbai's rainfall. Thus by connecting with all the analysis done through this paper, it can be said that convective rainfall dominates the pre-monsoon period over orographic station, with convectivity becoming evident at rain rates greater than 16 mm/h. On the other hand, during the monsoon period, local thermodynamic conditions and higher moisture availability trigger the formation of deep convective clouds over coastal areas, thereby resulting for more convective rainfall in the coastal city compared to the orographic station.
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.