Polarization models of young stellar objects – II. Linear and circular polarimetry of R Coronae Australis     

Stuart Clark  Alan McCall  Antonio Chrysostomou  Tim Gledhill  Jeremy Yates  James Hough 《Monthly notices of the Royal Astronomical Society》2000,319(2):337-349

Near-infrared linear imaging polarimetry of the young stellar objects R CrA and T CrA in the J , H and K n bands, and circular imaging polarimetry in the H band, is presented. The data are modelled with the Clark and McCall scattering model. The R CrA and T CrA system is shown to be a particularly complex scattering environment. In the case of R CrA there is evidence that the wavelength dependence of polarization changes across the nebula. MRN dust grain models do not explain this behaviour. Depolarization by line emission is considered as an alternative explanation. The dust grain properties could also be changing across the nebula.
Although surrounded by reflection nebulosity, there is a region of particularly low polarization surrounding R CrA that is best modelled by the canonical bipolar outflow being truncated by an evacuated spherical cavity surrounding the star. The symmetry axis of the nebula appears inclined by 50° to the plane of the sky.
The H -band circular polarimetry of R CrA clearly shows a quadrupolar structure of positive and negative degrees of circular polarization that reach peak magnitudes of ∼5 per cent within our limited map. It is shown that spherical MRN grains are incapable of producing this circular polarization given the observed linear polarization of the R CrA system. Instead, scattering from aligned non-spherical grains is proposed as the operating mechanism.
T CrA is a more archetypical bipolar reflection nebula, and this object is modelled as a canonical parabolic reflection nebula that lies in the plane of the sky. The wavelength independence of linear polarization in the T CrA reflection nebula suggests that the scattering particles are Rayleigh sized. This is modelled with the MRN interstellar grain size distribution.  相似文献   

Multi-frequency electromagnetic method for inductive measurement of ground induced polarization and resistivity     

Carlos Alberto Dias  Hédison Kiuity Sato  Marcos Vitor Barbosa Machado  Olivar Antonio Lima de Lima 《Geophysical Prospecting》2019,67(1):210-225

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A New TanSat XCO_2 Global Product towards Climate Studies     

Dongxu YANG  Yi LIU  Hartmut BOESCH  Lu YAO  Antonio DI NOIA  Zhaonan CAI  Naimeng LU  Daren LYU  Maohua WANG  Jing WANG  Zengshan YIN  Yuquan ZHENG 《大气科学进展》2021,38(1):8-11

The 1st Chinese carbon dioxide(CO2)monitoring satellite mission,TanSat,was launched in 2016.The 1st TanSat global map of CO2 dry-air mixing ratio(XCO2)measurements over land was released as version 1 data product with an accuracy of 2.11 ppmv(parts per million by volume).In this paper,we introduce a new(version 2)TanSat global XCO2 product that is approached by the Institute of Atmospheric Physics Carbon dioxide retrieval Algorithm for Satellite remote sensing(IAPCAS),and the European Space Agency(ESA)Climate Change Initiative plus(CCI+)TanSat XCO2 product by University of Leicester Full Physics(UoL-FP)retrieval algorithm.The correction of the measurement spectrum improves the accuracy(?0.08 ppmv)and precision(1.47 ppmv)of the new retrieval,which provides opportunity for further application in global carbon flux studies in the future.Inter-comparison between the two retrievals indicates a good agreement,with a standard deviation of 1.28 ppmv and a bias of?0.35 ppmv.  相似文献   

Spatial and environmental analysis of an ostracod metacommunity from endorheic lakes     

Andreu Castillo-Escrivà  Luis Valls  Carlos Rochera  Antonio Camacho  Francesc Mesquita-Joanes 《Aquatic Sciences - Research Across Boundaries》2016,78(4):707-716

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Monitoring crater-wall collapse at active volcanoes: a study of the 12 January 2013 event at Stromboli     

Sonia Calvari  Emanuele Intrieri  Federico Di Traglia  Alessandro Bonaccorso  Nicola Casagli  Antonio Cristaldi 《Bulletin of Volcanology》2016,78(5):39

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Reconstructing eruptive source parameters from tephra deposit: a numerical study of medium-sized explosive eruptions at Etna volcano     

Antonio Spanu  Mattia de’ Michieli Vitturi  Sara Barsotti 《Bulletin of Volcanology》2016,78(9):59

Since the 1970s, multiple reconstruction techniques have been proposed and are currently used, to extrapolate and quantify eruptive parameters from sampled tephra fall deposit datasets. Atmospheric transport and deposition processes strongly control the spatial distribution of tephra deposit; therefore, a large uncertainty affects mass derived estimations especially for fall layer that are not well exposed. This paper has two main aims: the first is to analyse the sensitivity to the deposit sampling strategy of reconstruction techniques. The second is to assess whether there are differences between the modelled values for emitted mass and grainsize, versus values estimated from the deposits. We find significant differences and propose a new correction strategy. A numerical approach is demonstrated by simulating with a dispersal code a mild explosive event occurring at Mt. Etna on 24 November 2006. Eruptive parameters are reconstructed by an inversion information collected after the eruption. A full synthetic deposit is created by integrating the deposited mass computed by the model over the computational domain (i.e., an area of 7.5 × 10⁴ km ²). A statistical analysis based on 2000 sampling tests of 50 sampling points shows a large variability, up to 50 % for all the reconstruction techniques. Moreover, for some test examples Power Law errors are larger than estimated uncertainty. A similar analysis, on simulated grain-size classes, shows how spatial sampling limitations strongly reduce the utility of available information on the total grain size distribution. For example, information on particles coarser than ?(?4) is completely lost when sampling at 1.5 km from the vent for all columns with heights less than 2000 m above the vent. To correct for this effect an optimal sampling strategy and a new reconstruction method are presented. A sensitivity study shows that our method can be extended to a wide range of eruptive scenarios including those in which aggregation processes are important. The new correction method allows an estimate of the deficiency for each simulated class in calculated mass deposited, providing reliable estimation of uncertainties in the reconstructed total (whole deposit) grainsize distribution.  相似文献   

Suitability of energy cone for probabilistic volcanic hazard assessment: validation tests at Somma-Vesuvius and Campi Flegrei (Italy)     

Pablo Tierz  Laura Sandri  Antonio Costa  Lucia Zaccarelli  Mauro Antonio Di Vito  Roberto Sulpizio  Warner Marzocchi 《Bulletin of Volcanology》2016,78(11):79

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Structure of Alluvial Valleys from 3-D Gravity Inversion: The Low Andarax Valley (Almería,Spain) Test Case     

Antonio G. Camacho  Enrique Carmona  Antonio García-Jerez  Francisco Sánchez-Martos  Juan F. Prieto  José Fernández  Francisco Luzón 《Pure and Applied Geophysics》2015,172(11):3107-3121

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An Overview of Geodetic Volcano Research in the Canary Islands     

José Fernández  Pablo J. González  Antonio G. Camacho  Juan F. Prieto  Guadalupe Brú 《Pure and Applied Geophysics》2015,172(11):3189-3228

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Classifying the flow regimes of Mediterranean streams using multivariate analysis   总被引：1，自引：0，他引：1       下载免费PDF全文

Ons Oueslati  Anna Maria De Girolamo  Aziz Abouabdillah  Thomas R. Kjeldsen  Antonio Lo Porto 《水文研究》2015,29(22):4666-4682

Rivers in the Mediterranean region often exhibit an intermittent character. An understanding and classification of the flow regimes of these rivers is needed, as flow patterns control both physicochemical and biological processes. This paper reports an attempt to classify flow regimes in Mediterranean rivers based on hydrological variables extracted from discharge time series. Long‐term discharge records from 60 rivers within the Mediterranean region were analysed in order to classify the streams into different flow regime groups. Hydrological indices (HIs) were derived for each stream and principal component analysis (PCA) and then applied to these indices to identify subsets of HIs describing the major sources of variations, while simultaneously minimizing redundancy. PCA was performed for two groups of streams (perennial and temporary) and for all streams combined. The results show that whereas perennial streams are mainly described by high‐flow indices, temporary streams are described by duration, variability and predictability indices. Agglomerative cluster analysis based on HIs identified six groups of rivers classified according to differences in intermittency and variability. A methodology allowing such a classification for ungauged catchments was also tested. Broad‐scale catchment characteristics based on digital elevation, climate, soil and land use data were derived for each long‐term station where these data were available. By using stepwise multiple regression analysis, statistically significant relationships were fitted, linking the three selected hydrological variables (mean annual number of zero‐flow days, predictability and flashiness) to the catchment characteristics. The method provides a means of simplifying the complexity of river systems and is thus useful for river basin management. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献