Diurnal Variations of Precipitation over the Steep Slopes of the Himalayas Observed by TRMM PR and VIRS

This study investigates diurnal variations of precipitation during May–August, 1998–2012, over the steep slopes of the Himalayas and adjacent regions (flat Gangetic Plains–FGP, foothills of the Himalayas–FHH, the steep slope of the southern Himalayas–SSSH, and the Himalayas-Tibetan Plateau tableland...

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Veröffentlicht in:Advances in atmospheric sciences 2021-04, Vol.38 (4), p.641-660
Hauptverfasser: Pan, Xiao, Fu, Yunfei, Yang, Sen, Gong, Ying, Li, Deqin
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Fu, Yunfei
Yang, Sen
Gong, Ying
Li, Deqin
description This study investigates diurnal variations of precipitation during May–August, 1998–2012, over the steep slopes of the Himalayas and adjacent regions (flat Gangetic Plains–FGP, foothills of the Himalayas–FHH, the steep slope of the southern Himalayas–SSSH, and the Himalayas-Tibetan Plateau tableland–HTPT). Diurnal variations are analyzed at the pixel level utilizing collocated TRMM precipitation radar and visible infrared data. The results indicate that rain parameters (including rain frequency, rain rate, and storm top altitude) are predominantly characterized by afternoon maxima and morning minima at HTPT and FGP, whereas, maximum rain parameters at FHH typically occur in the early morning. Rain parameters at SSSH are characterized by double peaks; one in the afternoon and one at midnight. Over HTPT and FGP, convective activity is strongest in the afternoon with the thickest crystallization layer. Over FHH, the vertical structure of precipitation develops most vigorously in the early morning when the most intense collision and growth of precipitation particles occurs. Over SSSH, moist convection is stronger in the afternoon and at midnight with strong mixing of ice and water particles. The results of harmonic analysis show that rain bands move southward from lower elevation of SSSH to FHH with apparent southward propagation of the harmonic phase from midnight to early morning. Moreover, the strongest diurnal harmonic is located at HTPT, having a diurnal harmonic percentage variance of up to 90%. Large-scale atmospheric circulation patterns exhibit obvious diurnal variability and correspond well to the distribution of precipitation.
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Diurnal variations are analyzed at the pixel level utilizing collocated TRMM precipitation radar and visible infrared data. The results indicate that rain parameters (including rain frequency, rain rate, and storm top altitude) are predominantly characterized by afternoon maxima and morning minima at HTPT and FGP, whereas, maximum rain parameters at FHH typically occur in the early morning. Rain parameters at SSSH are characterized by double peaks; one in the afternoon and one at midnight. Over HTPT and FGP, convective activity is strongest in the afternoon with the thickest crystallization layer. Over FHH, the vertical structure of precipitation develops most vigorously in the early morning when the most intense collision and growth of precipitation particles occurs. Over SSSH, moist convection is stronger in the afternoon and at midnight with strong mixing of ice and water particles. The results of harmonic analysis show that rain bands move southward from lower elevation of SSSH to FHH with apparent southward propagation of the harmonic phase from midnight to early morning. Moreover, the strongest diurnal harmonic is located at HTPT, having a diurnal harmonic percentage variance of up to 90%. Large-scale atmospheric circulation patterns exhibit obvious diurnal variability and correspond well to the distribution of precipitation.</description><identifier>ISSN: 0256-1530</identifier><identifier>EISSN: 1861-9533</identifier><identifier>DOI: 10.1007/s00376-020-0246-9</identifier><language>eng</language><publisher>Heidelberg: Science Press</publisher><subject>Atmospheric circulation ; Atmospheric circulation patterns ; Atmospheric precipitations ; Atmospheric Sciences ; Convection ; Convective activity ; Crystallization ; Diurnal variations ; Earth and Environmental Science ; Earth Sciences ; Elevation ; Foothills ; Fourier analysis ; Geophysics/Geodesy ; Harmonic analysis ; Infrared radar ; Maxima ; Meteorology ; Moist convection ; Original Paper ; Parameters ; Plateaus ; Precipitation ; Radar ; Radar data ; Rain ; Rainfall frequency ; Slopes ; Storms ; TRMM satellite ; Tropical Rainfall Measuring Mission (TRMM) ; Vertical profiles</subject><ispartof>Advances in atmospheric sciences, 2021-04, Vol.38 (4), p.641-660</ispartof><rights>Institute of Atmospheric Physics/Chinese Academy of Sciences, and Science Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021</rights><rights>Institute of Atmospheric Physics/Chinese Academy of Sciences, and Science Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021.</rights><rights>Copyright © Wanfang Data Co. 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Atmos. Sci</addtitle><description>This study investigates diurnal variations of precipitation during May–August, 1998–2012, over the steep slopes of the Himalayas and adjacent regions (flat Gangetic Plains–FGP, foothills of the Himalayas–FHH, the steep slope of the southern Himalayas–SSSH, and the Himalayas-Tibetan Plateau tableland–HTPT). Diurnal variations are analyzed at the pixel level utilizing collocated TRMM precipitation radar and visible infrared data. The results indicate that rain parameters (including rain frequency, rain rate, and storm top altitude) are predominantly characterized by afternoon maxima and morning minima at HTPT and FGP, whereas, maximum rain parameters at FHH typically occur in the early morning. Rain parameters at SSSH are characterized by double peaks; one in the afternoon and one at midnight. Over HTPT and FGP, convective activity is strongest in the afternoon with the thickest crystallization layer. 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Fu, Yunfei ; Yang, Sen ; Gong, Ying ; Li, Deqin</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c416t-3a1728cef9ba1c548704e19c0dc7b656fa2b4140aa81a14647c87cc9568debf43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Atmospheric circulation</topic><topic>Atmospheric circulation patterns</topic><topic>Atmospheric precipitations</topic><topic>Atmospheric Sciences</topic><topic>Convection</topic><topic>Convective activity</topic><topic>Crystallization</topic><topic>Diurnal variations</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Elevation</topic><topic>Foothills</topic><topic>Fourier analysis</topic><topic>Geophysics/Geodesy</topic><topic>Harmonic analysis</topic><topic>Infrared radar</topic><topic>Maxima</topic><topic>Meteorology</topic><topic>Moist convection</topic><topic>Original Paper</topic><topic>Parameters</topic><topic>Plateaus</topic><topic>Precipitation</topic><topic>Radar</topic><topic>Radar data</topic><topic>Rain</topic><topic>Rainfall frequency</topic><topic>Slopes</topic><topic>Storms</topic><topic>TRMM satellite</topic><topic>Tropical Rainfall Measuring Mission (TRMM)</topic><topic>Vertical profiles</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pan, Xiao</creatorcontrib><creatorcontrib>Fu, Yunfei</creatorcontrib><creatorcontrib>Yang, Sen</creatorcontrib><creatorcontrib>Gong, Ying</creatorcontrib><creatorcontrib>Li, Deqin</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; 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Atmos. Sci</stitle><date>2021-04-01</date><risdate>2021</risdate><volume>38</volume><issue>4</issue><spage>641</spage><epage>660</epage><pages>641-660</pages><issn>0256-1530</issn><eissn>1861-9533</eissn><abstract>This study investigates diurnal variations of precipitation during May–August, 1998–2012, over the steep slopes of the Himalayas and adjacent regions (flat Gangetic Plains–FGP, foothills of the Himalayas–FHH, the steep slope of the southern Himalayas–SSSH, and the Himalayas-Tibetan Plateau tableland–HTPT). Diurnal variations are analyzed at the pixel level utilizing collocated TRMM precipitation radar and visible infrared data. The results indicate that rain parameters (including rain frequency, rain rate, and storm top altitude) are predominantly characterized by afternoon maxima and morning minima at HTPT and FGP, whereas, maximum rain parameters at FHH typically occur in the early morning. Rain parameters at SSSH are characterized by double peaks; one in the afternoon and one at midnight. Over HTPT and FGP, convective activity is strongest in the afternoon with the thickest crystallization layer. Over FHH, the vertical structure of precipitation develops most vigorously in the early morning when the most intense collision and growth of precipitation particles occurs. Over SSSH, moist convection is stronger in the afternoon and at midnight with strong mixing of ice and water particles. The results of harmonic analysis show that rain bands move southward from lower elevation of SSSH to FHH with apparent southward propagation of the harmonic phase from midnight to early morning. Moreover, the strongest diurnal harmonic is located at HTPT, having a diurnal harmonic percentage variance of up to 90%. Large-scale atmospheric circulation patterns exhibit obvious diurnal variability and correspond well to the distribution of precipitation.</abstract><cop>Heidelberg</cop><pub>Science Press</pub><doi>10.1007/s00376-020-0246-9</doi><tpages>20</tpages></addata></record>
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subjects Atmospheric circulation
Atmospheric circulation patterns
Atmospheric precipitations
Atmospheric Sciences
Convection
Convective activity
Crystallization
Diurnal variations
Earth and Environmental Science
Earth Sciences
Elevation
Foothills
Fourier analysis
Geophysics/Geodesy
Harmonic analysis
Infrared radar
Maxima
Meteorology
Moist convection
Original Paper
Parameters
Plateaus
Precipitation
Radar
Radar data
Rain
Rainfall frequency
Slopes
Storms
TRMM satellite
Tropical Rainfall Measuring Mission (TRMM)
Vertical profiles
title Diurnal Variations of Precipitation over the Steep Slopes of the Himalayas Observed by TRMM PR and VIRS
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