Abstract
The P-band synthetic aperture radar of the European Space Agency BIOMASS mission will be affected by ionospheric phase scintillation at high latitudes, which introduces a random high-order azimuth phase error. The dependence of the performance of the phase gradient autofocus (PGA) algorithm for scintillation compensation on the strength of ionospheric turbulence and the signal-to-clutter ratio (SCR) is analyzed. In order to keep resolution degradation below 2%, the SCR must exceed 16 and 20 dB for turbulence strengths CkL=1033 and 1034, respectively. For large values of CkL, phase scintillation adds significantly to post-PGA degradation in the integrated and peak sidelobe ratios. Simulations based on scenes derived from PALSAR data demonstrate the effectiveness of PGA.
| Original language | English |
|---|---|
| Article number | 7047673 |
| Pages (from-to) | 1367-1371 |
| Number of pages | 5 |
| Journal | IEEE Geoscience and Remote Sensing Letters |
| Volume | 12 |
| Issue number | 6 |
| DOIs | |
| State | Published - Jun 2015 |
Keywords
- Image quality
- ionospheric phase scintillation
- phase gradient autofocus (PGA)
- synthetic aperture radar (SAR)
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