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Height Assignment Improvement in Kalpana-1 Atmospheric Motion Vectors

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Abstract

The real-time operational use of atmospheric motion vectors (AMVs) at numerical weather prediction (NWP) centers in India are being adversely affected due to inaccurate height assignment of cloud tracers, especially in thin semi-transparent clouds. In India, the operational derivation of AMVs from the Indian geostationary satellite Kalpana-1 began few years ago. A statistical empirical method (SEM) of height assignment, based on a genetic algorithm, is currently used to estimate the height of the retrieved vectors from Kalpana-1. This method has many limitations. In this paper, attempts have been made to implement the widely used and well tested height assignment methods such as the infrared window (WIN) technique, the H2O intercept, and the cloud base method in the Kalpana-1 AMV retrieval algorithm. The new height assignment algorithm significantly improves the statistics of the retrieved winds when compared to radiosondes, especially in high and mid levels winds.

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Acknowledgments

The authors are thankful to the anonymous reviewers for their critical and insightful comments and suggestions which have significantly improved the quality and presentation of the current version of the manuscript. The first author (SKD) thankfully acknowledges the financial support from M/S Antrix Corporation Limited, the commercial wing of the Indian Space Research Organization (ISRO), Department of Space, Govt. of India, for this study. The authors are also thankful to Shri A. S. Kiran Kumar, the Director, SAC for critical comments and suggestions during the course of this work. The encouragement and help from the Deputy Director, EPSA SAC, ISRO Ahmedabad is also acknowledged.

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Correspondence to S. K. Deb.

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Deb, S.K., Wanzong, S., Velden, C.S. et al. Height Assignment Improvement in Kalpana-1 Atmospheric Motion Vectors. J Indian Soc Remote Sens 42, 679–687 (2014). https://doi.org/10.1007/s12524-013-0278-z

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  • DOI: https://doi.org/10.1007/s12524-013-0278-z

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