This work is focused on the forthcoming ROSE-L mission, developed by the European Space Agency (ESA) as part of the Copernicus Expansion Programme. Among the different advanced engineering solutions that will be exploited by the system, we concentrate on the ScanSAR acquisition mode and show how to enable ROSE-L for a high gain two-look configuration. More specifically, we propose a solution aimed at achieving different goals.The first goal is focused on better tailoring the ROSE-L system, originally designed for a one-look ScanSAR mode configuration, to a more attractive two-look one. The second goal is to retain the azimuth resolution and the range swath of the original system design. The third goal is to be compliant with the main system specifications, with respect to the one- look mode configuration.To achieve these goals, we propose to properly shape the radiated azimuth beam, without upsetting the original design of the ROSE-L radar antenna and taking advantage of the degrees of freedom offered by its current layout.

This work shows that additional ScanSAR capabilities, with respect to those achievable through the current synthetic aperture radar (SAR) system of the forthcoming Radar Observation System for Europe at L-band (ROSE-L) mission, may be easily enabled through a proper shaping of the azimuth pattern of the TX radar antenna. In particular, we show that by properly acting only on the distribution of the input excitations of the elements of the currently designed TX antenna array, we can move from a single azimuth-look ScanSAR configuration to a more attractive two-look one. This result is achieved without upsetting the current system architecture and without changing the current mission parameters [such as azimuth resolution, range swath, and pulse repetition frequency (PRF)], all tailored to a one-look ScanSAR configuration. On the other hand, the proposed two-look mode requires to double the azimuth beamwidth with respect to the one-look mode, thus leading to an unavoidable antenna gain decrease, whose amount is approximately 3 dB. The presented analysis also shows that, by still acting on the distribution of the input excitations of the TX antenna array, the scalloping effect can be significantly mitigated with respect to that of the current system design, in both scenarios relevant to the original one-look ScanSAR configuration and the proposed two-look one.

The "Multi-mission and multi-frequency SAR" program (2021-2023) of the Italian Space Agency supported the national community to develop algorithms combining SAR data collected in C, X and L-bands. Main achievements in terms of SAR data exploitation, integration and data fusion, and new products prototyping are presented with regard to agriculture, natural hazards, urban areas, cryosphere, sea and coast. Perspectives are finally outlined with regard to future SAR missions and towards downstream applications.

In the future ROSE-L mission, supported by the European Space Agency (ESA) as part of the Copernicus Expansion Programme, different advanced acquisition techniques will be simultaneously experienced, namely, ScanSAR, Scan On Receive and Digital Beam Forming on receive. This work shows that additional ScanSAR capabilities with respect to those achievable through the current ROSE-L system design may be enabled through proper shaping of the azimuth pattern of the TX radar antenna. In particular, we show that without upsetting the current system architecture, and properly acting only on the distribution of the input excitations of the elements of the currently designed TX array antenna, we can obtain a significant mitigation of the scalloping effect and/or move from a single azimuth look ScanSAR configuration to a more attractive two-look one.

In continuity with the investments made on SAR technologies in the last two decades by the Italian Space Agency (ASI), the “Multi-mission and multi-frequency SAR” program currently supports ten R&D projects aiming to design, develop and test innovative algorithms for exploitation of multi-mission/multi-frequency SAR data. Perspectives of engineering and pre-operational development are demonstrated with regard to various application domains (i.e. agriculture, urban areas, natural hazards, cryosphere, sea and coast). Access to COSMO-SkyMed and SAOCOM images is facilitated by ASI to allow the research consortia to achieve an effective multi-frequency SAR data integration. The program represents a foundational step in the ASI's roadmap towards “scientific downstream applications”, i.e. applications enabled by the exploitation of mature and validated algorithms that have been originally developed to answer scientific questions and/or retrieve geophysical parameters, and have been brought to the stage that they can generate products that address specific user needs beyond scientific and academic purposes only.

Abstract The China Seismo‐Electromagnetic Satellite (CSES) space mission—also known as Limadou in Italian—is a scientific collaboration between China and Italy that aims to investigate the structure and dynamics of the iono/magnetosphere, and in particular to study the possible correlation of perturbations to the occurrence of high‐magnitude seismic events. The Chinese satellite houses the Italian high‐energy particle detector (HEPD), an apparatus composed of a silicon tracker and a calorimeter system, which detects electrons and protons in the energy ranges 3–100 and 30–200 MeV, respectively. The satellite was launched on February 2, 2018; after a commissioning phase dedicated to the setting of an optimal configuration, HEPD is fully operational since July 28, 2018. After a general overview of the CSES‐Limadou mission, this article presents the structure of the HEPD apparatus and describes the design and implementation of the software for the embedded computer system that is responsible for HEPD management. The onboard software runs on the digital signal processors of two electronic boards (CPU and data acquisition), monitors system status, handles instrument data acquisition, performs periodic calibration of the subdetectors, performs data compression, and communicates with the satellite. An overview of HEPD in‐flight operations and performance is given in the last section.

Recently, the Italian Space Agency (ASI) and the Jet Propulsion Laboratory (JPL) have agreed to carry out a joint study for an Earth Observation scientific mission in the infrared spectral range (MWIR-LWIR). A mission of this type is considered of high priority by the NASA's “Decadal Survey” plan, as well as being one of the priorities of the future Sentinel of the Copernicus program. Furthermore, an MWIR-LWIR system with spatial resolutions better than 90 m (target 50 m) could represent a formidable integration of the observational capacity of the ASI PRISMA and SHALOM missions, as it would allow observing the entire wavelength range from Visible to thermal IR and consequently expanding the spectrum of scientific applications of the national satellite system. INGV in 2018-2019 in the frame of ASI contract has carried out a review of scientific and technical requirements for a new EO “Thermal Mission” which my support a large number of applications.

Globally, 800 million people live within 100 km of a volcano thought to have been active in the last 10,000 years. The basis of forecasting the short term progression of volcanic unrest or onset of eruption is high quality monitoring data, ideally analysed in near real time consistently over long time periods. Volcanic deformation – the displacement of the Earth's surface in response to magmatic or volcanic processes – forms the foundation of many monitoring streams in combination with measurements of seismicity and gas emission. At present, < 10% of Holocene volcanoes are monitored routinely, while up to 45% are not monitored at all.

The monitoring of the recovery phase in the aftermath of an emergency scenario is tackled in this paper in terms of a change-detection perspective and through the integration of multisensor, multisource, and contextual information associated with high resolution optical and SAR data. The method makes use of the Markov random field theory to integrate the spatial context and the temporal correlation associated with images acquired at different dates. Moreover, the adoption of a region-based approach allows the characterization of the geometrical structures in the images through the employment of multiple segmentation maps at different scales. The performances of the proposed approach are evaluated on pairs of COSMO-SkyMed/Pléiades images acquired over Haiti in the aftermath of Hurricane Matthew.

This paper describes two examples of synergistic management of EO based services for flood emergency monitoring. The first relates to the benefits of collaboration between decision makers, end users and experts reporting the case of the November 2014 Liguria and Po River flooding, when early activation, prior to the occurrence of the flood, was made possible and the second shows the benefits of the synergy between Sentinel-1 (S-1) and COSMO-SkyMed (CSK) contributing missions for monitoring floods at national scale. The two examples are referred to flood monitoring but the conclusions can be easily extended to other risks.

The present paper reports on some insights in the use of Synthetic Aperture Radars (SAR) for bathymetric data retrieval by exploiting variation in swell wave parameters approaching the shoreline. Since SAR signals are unable to penetrate sea surface and to reach seabed, echoed signals from sea surface are used to investigate underwater bathymetry in coastal area. A suitable data processing methodology is proposed to properly detect swell shoaling and refraction phenomena, and to accurately measure swell parameters. The described methodology is tested by using ALOS L-band SAR images over the Gulf of Naples, Italy. A Digital Elevation Model (DEM) of the investigated area is thus obtained. Results are consistent with the values reported in the Official Nautical Chart provided by the Italian Navy Hydrographic Institute.

The SAP4PRISMA is a four year research project which aims at developing algorithms and products for the future PRISMA mission. The project started on May 2010 and is now entering his full activities as the ”PRISMA like” data set has been defined and the test areas were selected. The paper describes the main project objectives and the activities realized in the first 9 months of the project.

We used a variety of SAR-based techniques to measure the crustal deformation associated to the Darfield and Christchurch earthquakes, New Zealand. We detected clear post-seismic signals of the Darfield earthquake, and a pre-seismic signal spatially and temporally associated to the Christchurch earthquake. The small pre-seismic signal (∼25 mm) has an opposite polarity of the much larger co-seismic one (∼150 mm) in the same area.

Volcanic plumes represent a visible indicator of volcanic activity. They vary in space and time, strongly influenced by the quiescent or eruptive status of the volcano. Different volcanic activities, such as volcanic clouds and plumes, inject into the atmosphere gases and aerosol at different latitudes, altitudes and with different times of residence. Released by the magma, plumes are a turbulent mixture of gases, solid particles and liquid droplets, emitted at high temperature continuously from summit craters, fumarolic fields or during eruptive episodes. Mt. Etna, in Sicily (Italy), is one of the world's most frequent emitters of volcanic plumes. It show a permanent degassing plumes periodically interrupted by copious tephra emission and fallout that damage the inhabited and cultivated areas and created serious hazards to air traffic, as volcanic clouds can spread thousand of km in the central Mediterranean area. Recurrent closures of the Catania International airport have often been necessary, causing great losses to the local economy (Andronico et al 2009). For these reasons Mt. Etna is continually monitored and recent a new approach has been adapted integrating ground network data with the analysis of space data. In order to extract geophysical parameters related to volcano status software modules has been developed divided by early warning phase, crisis phase and post- crisis phase. Modules using already developed remote sensing techniques in the VIS and IR wavelength range. Here we present two modules for the Mt. Etna volcanic plume analysis using ASTER on TERRA and HYPERION on EO-1 data. This study is carried out within the SRV project, funded by the Italian Space Agency (ASI).

SIGRIS (SIstema di osservazione spaziale per la Gestione del RIschio Sismico) is a pilot project aiming to the realization of a system, based on satellite remote sensing data, for the seismic risk management. The project is funded by the Italian Space Agency (ASI). ASI is deeply interested on the development of new applications, using satellite data, dedicated to the monitoring and management of the natural hazards. SIGRIS is focused on providing the information services for mapping, monitoring, forecasting and awareness of seismic risk. The Earth Observation products are generated by using GPS data, optical and SAR (Synthetic Aperture Radar) images. This project deals with the data exploitation of the new Italian Earth Observation mission: COSMO-SkyMed, a constellation of four satellites equipped with an X-band high resolution SAR.