2016
DOI: 10.1002/qj.2929
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Assimilation of INSAT‐3D hydro‐estimator method retrieved rainfall for short‐range weather prediction

Abstract: India launched a geostationary satellite INSAT-3D on 26 July 2013 with an objective to monitor the Earth's surface using various spectral channels of meteorological importance. INSAT-3D retrieved Hydro-Estimator (HE) rainfall is compared with Tropical Rainfall Measuring Mission (TRMM) 3B42 V7 merged rainfall and in situ observations from the India Meteorological Department (IMD). Results suggest that INSAT-3D HE rainfall is of reasonably good quality and hence can be used for various meteorological application… Show more

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Cited by 51 publications
(27 citation statements)
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“…The Yonsei State University (Hong & Dudhia, ; Hong & Pan, ) scheme is used for planetary boundary layers that take care of vertical subgrid‐scale fluxes due to eddy transports in the full atmospheric column. These physics parameterization schemes have been tested over the Indian region in earlier studies (Kumar et al, ; Kumar & Varma, ).…”
Section: Model Description and Methodologymentioning
confidence: 99%
“…The Yonsei State University (Hong & Dudhia, ; Hong & Pan, ) scheme is used for planetary boundary layers that take care of vertical subgrid‐scale fluxes due to eddy transports in the full atmospheric column. These physics parameterization schemes have been tested over the Indian region in earlier studies (Kumar et al, ; Kumar & Varma, ).…”
Section: Model Description and Methodologymentioning
confidence: 99%
“…Terrestial data are taken from the United States geological survey climatology. The details of the selected WRF model configurations are opted from Kumar and Varma (). Initially, total 92 particles are prepared with different combinations of 12 different cumulus parameterization (CP) schemes (viz., new eta Kain‐Fritsch scheme [CP1]; Betts‐Miller‐Janjic scheme [CP2]; Grell‐Freitas ensemble scheme [CP3]; Simplied Arakawa Schubert scheme [CP4]; Grell‐3D ensemble scheme [CP5]; Tiedtke scheme [CP6]; modified Kain‐Fritsch with trigger function [CP10]; Multiscale Kain‐Fritsch scheme [CP11]; new GFS simplified Arakawa‐Schubert scheme [CP14]; new Tiedtke scheme [CP16]; Grell‐Devenyi ensemble scheme [CP93]; old Kain‐Fritsch [CP99] schemes), four different microphysics (MP) schemes (viz., Eta [Ferrier; MP5]; WSM6 [MP6]; Goddard GCE scheme [MP7]; Thompson [MP8]), and two different planetary boundary layer (PBL) schemes (viz., YSU [PBL1]; MYNN2 [PBL5]) available in the WRF model (Skamarock et al, ).…”
Section: Wrf Modelmentioning
confidence: 99%
“…Terrestial data are taken from the United States geological survey climatology. The details of the selected WRF model configurations are opted from Kumar and Varma (2016…”
Section: Wrf Modelmentioning
confidence: 99%
“…Advanced WRF model simulations have been used to support observational results. The WRF model incorporates diverse physics schemes for the treatment of convection and mesoscale precipitation systems (Kumar & Shukla, 2019; Kumar & Varma, 2017). The WRF model set up, physical, and dynamical schemes used for present study are described in supporting information section 2.…”
Section: Data Sourcesmentioning
confidence: 99%