2011
DOI: 10.3390/a4030155
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Radio-Frequency Interference Detection and Mitigation Algorithms for Synthetic Aperture Radiometers

Abstract: The European Space Agency (ESA) successfully launched the Soil Moisture and Ocean Salinity (SMOS) mission in November 2, 2009. SMOS uses a new type of instrument, a synthetic aperture radiometer named MIRAS that provides full-polarimetric multi-angular L-band brightness temperatures, from which regular and global maps of Sea Surface Salinity (SSS) and Soil Moisture (SM) are generated. Although SMOS operates in a restricted band (1400–1427 MHz), radio-frequency interference (RFI) appears in SMOS imagery in many… Show more

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Cited by 56 publications
(21 citation statements)
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“…To identify contaminated pixels, we first apply the pixel-based SMOS RFI flags and subsequently identify remaining snapshots containing values above 300 K, which is outside of the geophysical range expected over polar oceans. Since RFI can either partly or completely destroy a snapshot [19], we remove the entire snapshot for simplicity, resulting in an increased data loss for these cases (see also Tian-Kunze et al [3]). …”
Section: Smosmentioning
confidence: 99%
“…To identify contaminated pixels, we first apply the pixel-based SMOS RFI flags and subsequently identify remaining snapshots containing values above 300 K, which is outside of the geophysical range expected over polar oceans. Since RFI can either partly or completely destroy a snapshot [19], we remove the entire snapshot for simplicity, resulting in an increased data loss for these cases (see also Tian-Kunze et al [3]). …”
Section: Smosmentioning
confidence: 99%
“…More details on the algorithm implementation can be found in [38]. Figure 4 shows the results of the proposed RFI detection/cancellation algorithm over real SMOS data acquired over the Caribbean sea: (a) the original brightness temperature image corrupted by a strong RFI, (b) the RFI "cleaned" brightness temperature; (c) the estimated RFI, and (d) the confidence of the RFI sources removed level (from 0 to 1, 0 being totally unreliable, and 1 being totally reliable).…”
Section: Radio Frequency Interference Detection and Mitigationmentioning
confidence: 99%
“…For the previous SMOS RFI detection methods using L1C data [8], [10], [15], the local maxima with BT > 350 K are selected as candidates of RFI spots. In the MUSIC pseudo-spectrum, local maxima are selected regardless of the spectrum values, i.e., a fixed threshold cannot be applied.…”
Section: F Local Peak Detectionmentioning
confidence: 99%
“…However, Radio-Frequency Interferences (RFI) have been detected since the first in-orbit measurements. RFI hamper the geophysical parameter retrieval in the affected pixels [5]- [8]. The interference nature in the impulse response of MIRAS makes contaminations even more serious [5], [7].…”
Section: Introductionmentioning
confidence: 99%
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