| タイトル | Interferometric synthetic aperture radar imagery of the Gulf Stream |
| 本文（外部サイト） | http://hdl.handle.net/2060/19950017519 |
| 著者（英） | Goldstein, R. M.; Foley, E. W.; Valenzuela, G. R.; Jansen, R. W.; Ainsworth, T. L.; Chubb, S. R.; Cannella, M. E.; Carande, R. E. |
| 著者所属（英） | Jet Propulsion Lab., California Inst. of Tech. |
| 発行日 | 1993-10-25 |
| 言語 | eng |
| 内容記述 | The advent of interferometric synthetic aperture radar (INSAR) imagery brought to the ocean remote sensing field techniques used in radio astronomy. Whilst details of the interferometry differ between the two fields, the basic idea is the same: Use the phase information arising from positional differences of the radar receivers and/or transmitters to probe remote structures. The interferometric image is formed from two complex synthetic aperture radar (SAR) images. These two images are of the same area but separated in time. Typically the time between these images is very short -- approximately 50 msec for the L-band AIRSAR (Airborne SAR). During this short period the radar scatterers on the ocean surface do not have time to significantly decorrelate. Hence the two SAR images will have the same amplitude, since both obtain the radar backscatter from essentially the same object. Although the ocean surface structure does not significantly decorrelate in 50 msec, surface features do have time to move. It is precisely the translation of scattering features across the ocean surface which gives rise to phase differences between the two SAR images. This phase difference is directly proportional to the range velocity of surface scatterers. The constant of proportionality is dependent upon the interferometric mode of operation. |
| NASA分類 | OCEANOGRAPHY |
| レポートNO | 95N23939 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/107807 |
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