2014
DOI: 10.1109/jstars.2014.2317287
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The COSMO-SkyMed Dual Use Earth Observation Program: Development, Qualification, and Results of the Commissioning of the Overall Constellation

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Cited by 38 publications
(21 citation statements)
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“…The single channel k-th image, acquired along the orbit with the orthogonal baseline k s' (see Figure 1), in a fixed pixel, is given by the integral superposition of the contributions of all the scatterers lying in the corresponding range-azimuth resolution cell, and located at different elevation coordinates s. A discrete estimate of γ can be found by ideally discretizing the integral operator. We can denote, with γ, the N × 1 column vector whose elements are the samples of the reflectivity at a fixed range and azimuth position, so the sampled received signal is related to γ by , = + u Φγ w (1) where u is an M × 1 observations column vector, w is an M × 1 column vector representing noise and clutter, and Φ is an M × N measurement matrix related to the acquisition geometry, whose generic element with index kl is given by We can denote, with γ, the N × 1 column vector whose elements are the samples of the reflectivity at a fixed range and azimuth position, so the sampled received signal is related to γ by…”
Section: Signal Modelmentioning
confidence: 99%
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“…The single channel k-th image, acquired along the orbit with the orthogonal baseline k s' (see Figure 1), in a fixed pixel, is given by the integral superposition of the contributions of all the scatterers lying in the corresponding range-azimuth resolution cell, and located at different elevation coordinates s. A discrete estimate of γ can be found by ideally discretizing the integral operator. We can denote, with γ, the N × 1 column vector whose elements are the samples of the reflectivity at a fixed range and azimuth position, so the sampled received signal is related to γ by , = + u Φγ w (1) where u is an M × 1 observations column vector, w is an M × 1 column vector representing noise and clutter, and Φ is an M × N measurement matrix related to the acquisition geometry, whose generic element with index kl is given by We can denote, with γ, the N × 1 column vector whose elements are the samples of the reflectivity at a fixed range and azimuth position, so the sampled received signal is related to γ by…”
Section: Signal Modelmentioning
confidence: 99%
“…A new class of SAR satellites, such as TerraSAR-X and TanDEM-X (X-band), COSMO-SkyMed (X-band), as well as Radarsat-2 (C-band), are providing images with resolution in the meter regime, and dual or full polarimetric SAR acquisition modes. In particular, the future second generation of COSMO-SkyMed will have full polarimetric SAR acquisition modes [1,2].…”
Section: Introductionmentioning
confidence: 99%
“…The main objective of this study is to fill this gap, by assessing the classification's improvement of VHR MS satellite images of a complex environment made up of both urban and rural areas by incorporating in the classification workflow single-polarization X-band SAR data, like CSK ® [32], without the need of developing ad hoc algorithms. The expected benefit of including the SAR information is to achieve a better knowledge of the LC/LU fragmentation.…”
Section: Integration Of Cosmo-skymed and Geoeye-1 Datamentioning
confidence: 99%
“…Some of these advantages are the increase of the mission flexibility and reliability, the reduction in costs, and the capability to survive possible failures by task exchanges among the platforms. The number of programs involving multiple spacecraft -either recently launched or under development -confirms the great interest for such a mission concept [1][2][3][4][5]. One of the challenges of these formations lies in the design of the techniques which allow the spacecraft to autonomously accomplish the tasks of guidance, navigation and control, both for translational and attitude dynamics.…”
Section: Introductionmentioning
confidence: 99%
“…The problems concerning the relative positions among spacecraft were widely investigated in the past [6,7], producing as a result a deep theoretic knowledge in this field [8]. On the other hand, the problem of attitude coordination among spacecraft is more recent, because strictly connected by the real implementation of mission utilizing distributed sensors [1,4]. Attitude coordination is an interesting and open field of research, as it does allow to imagine of new missions concepts for tracking moving or fixed objects in Earth, in orbit or in deep space.…”
Section: Introductionmentioning
confidence: 99%