Title
An Empirical Correction For The Mwr Brightness Temperature Smear Effect
Keywords
Aquarius/SAC-D; Brightness Temperature; empirical correction; MWR; radiometer; smear T anomaly B
Abstract
The Microwave Radiometer (MWR), on board of the SAC-D/Aquarius satellite, is a Dicke radiometer, operating at 23.8 and 36.5 GHz that was developed by Argentine Space Agency, CoNAE. Since the first earth surface TB images, there has been an anomalous effect when observing strong contrast radiometric scenes, such as land/water crossings. This effect is present in all push-broom beams and results in a 'smearing' of TB observations near high contrast areas. This paper presents the initial findings on this MWR brightness temperature anomaly that is best described as a coupling of sequential MWR feed horn measurements. In the present work, an empirical approach is used to mitigate this anomalous effect. © 2012 IEEE.
Publication Date
12-1-2012
Publication Title
International Geoscience and Remote Sensing Symposium (IGARSS)
Number of Pages
4680-4683
Document Type
Article; Proceedings Paper
Personal Identifier
scopus
DOI Link
https://doi.org/10.1109/IGARSS.2012.6350421
Copyright Status
Unknown
Socpus ID
84873173409 (Scopus)
Source API URL
https://api.elsevier.com/content/abstract/scopus_id/84873173409
STARS Citation
Farrar, Spencer; Labanda, Martin; Jacob, Maria Marta; Masuelli, Sergio; and Biswas, Sayak, "An Empirical Correction For The Mwr Brightness Temperature Smear Effect" (2012). Scopus Export 2010-2014. 3973.
https://stars.library.ucf.edu/scopus2010/3973