Improving Infrared-Based Precipitation Retrieval Algorithms Using Multi-Spectral Satellite Imagery
(Sprache: Englisch)
This thesis transforms satellite precipitation estimation through the integration of a multi-sensor, multi-channel approach to current precipitation estimation algorithms, and provides more accurate readings of precipitation data from space.
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This thesis transforms satellite precipitation estimation through the integration of a multi-sensor, multi-channel approach to current precipitation estimation algorithms, and provides more accurate readings of precipitation data from space.Using satellite data to estimate precipitation from space overcomes the limitation of ground-based observations in terms of availability over remote areas and oceans as well as spatial coverage. However, the accuracy of satellite-based estimates still need to be improved.
The approach introduced in this thesis takes advantage of the recent NASA satellites in observing clouds and precipitation. In addition, machine-learning techniques are also employed to make the best use of remotely-sensed "big data." The results provide a significant improvement in detecting non-precipitating areas and reducing false identification of precipitation.
Inhaltsverzeichnis zu „Improving Infrared-Based Precipitation Retrieval Algorithms Using Multi-Spectral Satellite Imagery “
- Introduction to the Current States of Satellite Precipitation Products- False Alarm in Satellite Precipitation Data
- Satellite Observations
- Reducing False Rain in Satellite Precipitation Products Using CloudSat Cloud Classification Maps and MODIS Multi-Spectral Images
- Integration of CloudSat Precipitation Profile in Reduction of False Rain
- Cloud Classification and its Application in Reducing False Rain
- Summary and Conclusions
Bibliographische Angaben
- Autor: Nasrin Nasrollahi
- 2014, 2015, XXI, 68 Seiten, 38 farbige Abbildungen, Masse: 16,3 x 24,4 cm, Gebunden, Englisch
- Verlag: Springer, Berlin
- ISBN-10: 3319120808
- ISBN-13: 9783319120805
Sprache:
Englisch
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