Abstract
A series of circle flights have been carried out over the sea surface, using the EMIRAD L-band polarimetric radiometer. Motion compensation is applied, and polarimetric azimuth signatures are generated. Single tracks show geophysical noise, typically about 2 K, but averaging decreases the noise, producing signatures with variations below 500 mK. A harmonic analysis of the results provides no clear signature, and for the 2nd, 3rd, and 4th Stokes parameters it is shown, that a significant part of the signal must be due to Gaussian noise. The 1st Stokes parameter is shown to have a 500 mK 2nd harmonic, but a comparison of the signature to the downwelling galactic background radiation indicates, that the signature may not origin from the wind driven sea surface pattern.
Original language | English |
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Title of host publication | IGARRS 2003 Proceedings of IEEE International Geoscience and Remote Sensing Symp, Toulouse, France |
Publisher | IEEE |
Publication date | 2003 |
Pages | 2738-2740 |
ISBN (Print) | 0-7803-7929-2 |
DOIs | |
Publication status | Published - 2003 |
Event | 2003 IEEE International Geoscience and Remote Sensing Symposium - Toulouse, France Duration: 21 Jul 2003 → 25 Jul 2003 http://ieeexplore.ieee.org/xpl/mostRecentIssue.jsp?punumber=9010 |
Conference
Conference | 2003 IEEE International Geoscience and Remote Sensing Symposium |
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Country/Territory | France |
City | Toulouse |
Period | 21/07/2003 → 25/07/2003 |
Internet address |