Surfaces and atmospheres of the outer planets, their satellites and ring systems     

Athena Coustenis  Sushil Atreya  Cécile Ferrari  Linda Spilker 《Planetary and Space Science》2008,56(1):1-2

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Huygens probe entry trajectory and attitude estimated simultaneously with Titan atmospheric structure by Kalman filtering     

Alessio Aboudan  Giacomo Colombatti  Francesca Ferri  Francesco Angrilli 《Planetary and Space Science》2008,56(5):573-585

Space probes entering planetary atmospheres are used for in situ study of their physical structures. During the entry phase aerodynamic forces exerted on the probe depend on atmospheric density. As a consequence accelerations measured by on-board sensors can be used to derive probe trajectory as well as atmospheric density, pressure and temperature profiles. In this work acceleration data acquired by the Huygens Atmospheric Structure Instrument (HASI) have been used to reconstruct the probe trajectory and the Titan's atmospheric structure from down to of altitude. An accurate six degree of freedom model of Huygens during the entry phase has been developed and a new reconstruction technique based on Kalman filtering is presented. This technique estimates simultaneously the probe trajectory, the attitude profile consistent with measured data and the atmospheric density, pressure and temperature.  相似文献   

Combining a rainfall–runoff model and a regionalization approach for flood and water resource assessment in the western Po Valley,Italy     

Alessio Cislaghi  Daniele Masseroni  Christian Massari  Stefania Camici  Luca Brocca 《水文科学杂志》2020,65(3):348-370

ABSTRACT

Selecting the best structure and parameterization of rainfall–runoff models is not straightforward and depends on a broad number of factors. In this study, the “Modello Idrologico Semi-Distribuito in continuo” (MISDc) was tested on 63 mountainous catchments in the western Po Valley (Italy) and the optimal model parameters were regionalized using different strategies. The model performance was evaluated through several indexes analysing hydrological regime, high-flow condition and flow–duration curve (FDC). In general, MISDc provides a good fit behaviour with a Kling-Gupta Efficiency index greater than 0.5 for 100% and 84% of cases for calibration and validation, respectively. Concerning the regionalization, spatial proximity approach is the most accurate solution obtaining satisfactory performance. Lastly, the predicted FDCs showed an excellent similarity with the observed ones. Results encourage to apply MISDc over the study area for flood forecasting and for assessing water resources availability thanks to the modest computational efforts and data requirements.  相似文献   

Exploiting spectral and spatial information in hyperspectral urban data with high resolution   总被引：2，自引：0，他引：2  

Dell'Acqua  F. Gamba  P. Ferrari  A. Palmason  J.A. Benediktsson  J.A. Arnason  K. 《Geoscience and Remote Sensing Letters, IEEE》2004,1(4):322-326

Very high resolution hyperspectral data should be very useful to provide detailed maps of urban land cover. In order to provide such maps, both accurate and precise classification tools need, however, to be developed. In this letter, new methods for classification of hyperspectral remote sensing data are investigated, with the primary focus on multiple classifications and spatial analysis to improve mapping accuracy in urban areas. In particular, we compare spatial reclassification and mathematical morphology approaches. We show results for classification of DAIS data over the town of Pavia, in northern Italy. Classification maps of two test areas are given, and the overall and individual class accuracies are analyzed with respect to the parameters of the proposed classification procedures.  相似文献   

Volcanic Tremor at Mt. Etna, Italy, Preceding and Accompanying the Eruption of July – August, 2001     

S. Falsaperla  S. Alparone  S. D'Amico  G. Di Grazia  F. Ferrari  H. Langer  T. Sgroi  S. Spampinato 《Pure and Applied Geophysics》2005,162(12):2583

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Zeolitization of Oligo-Miocene volcaniclastic rocks from Logudoro (northern Sardinia, Italy)   总被引：1，自引：0，他引：1  

Guido Cerri  Piergiulio Cappelletti  Alessio Langella  Maurizio de'Gennaro 《Contributions to Mineralogy and Petrology》2001,140(4):404-421

The present study reports the results of research on volcaniclastic products from Logudoro (northern Sardinia), a reconstructed stratigraphic succession some hundreds of meters thick, comprising two different ignimbritic units separated by an epiclastic layer (generally ˜10 m thick). Clinoptilolite is the most widely distributed authigenic phase in epiclastite and unwelded units, always associated with opal-CT and sometimes with smectite. An adularia-like feldspar, cristobalite and epigenetic quartz are typical phases of welded units. Within the zeolitized units (unwelded ignimbrite and epiclastic units) clinoptilolite and opal-CT constitute the cement deriving from the transformation of the precursor rhyolitic glass, in agreement with a single zeolitization process that developed after the deposition of the entire succession. Silica increases in zeolitized rocks with respect to the precursor material, leading to hypothesize that the secondary mineralization process was favored by mineralized hydrothermal fluids preferentially circulating through the fault system of the area. Quartz veins in welded subunit and K-feldspar (adularia-like) preferentially located near the faults are in agreement with this hypothesis. The interaction of these fluids with the glassy fraction favored its dissolution and the consequent crystallization of clinoptilolite. Furthermore, the pH increase and the silica supersaturation enhanced the contemporary or subsequent precipitation of opal-CT. Received: 5 June 2000 / Accepted: 14 August 2000  相似文献   

Pulsed high-energy radiation from oblique magnetic rotators     

A. Ferrari  E. Trussoni 《Astrophysics and Space Science》1975,33(1):111-126

A detailed analysis is reported of charged particle motion in the e.m. fields generated by oblique magnetic rotators. A full treatment of particle trajectories, radiated power and spectrum is given; astrophysical implications of these results in connection with pulsars, mainly NP 0532, are discussed and the possibility of a high energy pulsed radiation model with synchro-Compton emission at the speed-of-light cylinder is investigated.  相似文献   

Lunar gravity derived from long-period satellite motion — A proposed method     

A. J. Ferrari 《Celestial Mechanics and Dynamical Astronomy》1973,7(1):46-76

A new method has been devised to determine the spherical harmonic coefficients of the lunar gravity field. This method consists of a two-step data reduction and estimation process. In the first step, a weighted least-squares empirical orbit determination scheme is applied to Doppler tracking data from lunar orbits to estimate longpperiod Kepler elements and rates. Each of the Kepler elements is represented by an independent function of time. The long-period perturbing effects of the Earth, Sun, and solar radiation are explicitly modeled in this scheme. Kepler element variations estimated by this empirical processor are then ascribed to the non-central lunar gravitation features. Doppler data are reduced in this manner for as many orbits as are available. In the second step, the Kepler element rates are used as input to a second least-squares processor that estimates lunar gravity coefficients using the long-period Lagrange perturbation equations.Pseudo Doppler data have been generated simulating two different lunar orbits. This analysis included the perturbing effects of the L1 lunar gravity field, the Earth, the Sun, and solar radiation pressure. Orbit determinations were performed on these data and long-period orbital elements obtained. The Kepler element rates from these solutions were used to recover L1 lunar gravity coefficients. Overall results of this controlled experiment show that lunar gravity coefficients can be accurately determined and that the method is dynamically consistent with long-period perturbation theory.  相似文献   

On sky characterization of the BAORadio wide band digital backend     

R. Ansari  J. E. Campagne  P. Colom  C. Ferrari  Ch. Magneville  J. M. Martin  M. Moniez  A. S. Torrentó 《Experimental Astronomy》2016,41(1-2):117-144

We have observed regions of three galaxy clusters at z～[0.06÷0.09] (Abell85, Abell1205, Abell2440) with the Nançay radiotelescope (NRT) to search for 21 cm emission and to fully characterize the FPGA based BAORadio digital backend. We have tested the new BAORadio data acquisition system by observing sources in parallel with the NRT standard correlator (ACRT) back-end over several months. BAORadio enables wide band instantaneous observation of the [1250,1500] MHz frequency range, as well as the use of powerful RFI mitigation methods thanks to its fine time sampling. A number of questions related to instrument stability, data processing and calibration are discussed. We have obtained the radiometer curves over the integration time range [0.01,10 000] seconds and we show that sensitivities of few mJy over most of the wide frequency band can be reached with the NRT. It is clearly shown that in blind line search, which is the context of H _I intensity mapping for Baryon Acoustic Oscillations, the new acquisition system and processing pipeline outperforms the standard one. We report a positive detection of 21 cm emission at 3σ-level from galaxies in the outer region of Abell85 at ?1352 MHz (14400 km/s) corresponding to a line strength of ?0.8 Jy km/s. We also observe an excess power around ?1318 MHz (21600 km/s), although at lower statistical significance, compatible with emission from Abell1205 galaxies. Detected radio line emissions have been cross matched with optical catalogs and we have derived hydrogen mass estimates.  相似文献   

Quaternary adakite—Nb-enriched basalt association in the western Trans-Mexican Volcanic Belt: is there any slab melt evidence?     

Chiara M. Petrone  Luca Ferrari 《Contributions to Mineralogy and Petrology》2008,156(1):73-86

A spatial and temporal association between adakitic rocks and Nb-enriched basalts (NEB) is recognised for the first time in the western sector of the Trans-Mexican Volcanic Belt in the San Pedro–Cerro Grande Volcanic Complex (SCVC). The SCVC is composed of subalkalic intermediate to felsic rocks, spanning in composition from high-silica andesites to rhyolites, and by the young transitional hawaiite and mugearite lavas of Amado Nervo shield volcano. Intermediate to felsic rocks of the SCVC show many geochemical characteristics of typical adakites, such as high Sr/Y ratios (up to 180) and low Y (<18 ppm) and Yb contents. Mafic Amado Nervo rocks have high TiO₂ (1.5–2.3 wt%), Nb (14–27 ppm), Nb/La (0.5–0.9) and high absolute abundances of HFSE similar to those shown by NEB. However, the Sr and Nd isotopic signature of SCVC rocks is different from that shown by typical adakites and NEB. Although the adakites–NEB association has been traditionally considered as a strong evidence of slab-melting, we suggest that other processes can lead to its generation. Here, we show that parental magmas of adakitic rocks of the SCVC derive their adakitic characteristic from high-pressure crystal fractionation processes of garnet, amphibole and pyroxene of a normal arc basalt. On the other hand, Amado Nervo Na-alkaline parental magmas have been generated by sediment melting plus MORB-fluid flux melting of a heterogeneous mantle wedge, consisting of a mixture of depleted and an enriched mantle sources (90DM + 10EM). We cannot exclude a contribution to the subduction component of slab melts, because the component signature is dominated by sediment melt, but we argue that caution is needed in interpreting the adakites–NEB association in a genetic sense.  相似文献