Name
Abstract | ||
|---|---|---|
Sentinel-1 Cu0026D SAR instruments are designed to continue the observations beyond the lifetime of Sentinel-1 A u0026 B. They are to a high degree rebuilds of S-lAu0026B and will have the same imaging modes and interfaces to ground. Changes have been implemented within the SAR antenna by using a new Tile Amplifier design, which will contribute to improved radiometric stability and accuracy. The new tile amplifiers simplify the internal calibration approach by reducing the number of internal measurements from five to three. Another improvement is the introduction of interleaved noise measurements during image acquisition in addition to noise acquisitions in preamble and postamble. This is important as the surface brightness temperature have a significant impact on the acquired noise and can change the measured levels by up to 1 dB. A first tile for S-lC with the new design has been successfully tested. Results confirm the updated design and indicate improved measurement accuracy. |
Year | Venue | Field |
|---|---|---|
2018 | IGARSS | Preamble,Synthetic aperture radar,Computer science,Remote sensing,Radio frequency,Accuracy and precision,Tile,Temperature measurement,Calibration,Amplifier |
DocType | Citations | PageRank |
Conference | 0 | 0.34 |
References | Authors | |
0 | 7 | |
Name | Order | Citations | PageRank |
|---|---|---|---|
| Mathias von Alberti | 1 | 0 | 0.34 |
| Eberhard Schied | 2 | 0 | 0.34 |
| Siegmund Idler | 3 | 0 | 0.34 |
| Ignacio Navas Traver | 4 | 4 | 1.83 |
| Francisco Ceba Vega | 5 | 0 | 0.68 |
| Paul Snoeij | 6 | 0 | 0.34 |
| David Bibby | 7 | 0 | 1.01 |