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Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock

High Power Laser Science and Engineering 2018年第2期6卷 123-132页

作者： Th.Michel E.Falize B.Albertazzi g.rigon Y.Sakawa T.Sano H.Shimogawara R.Kumar T.Morita C.Michaut A.Casner R Barroso P.Mabey Y.Kuramitsu S.Laffite L.Van Box Som g.gregori R.Kodama N.Ozaki P.Tzeferacos D.Lamb M.Koenig luli-cnrs ecole polytechniquecea:universite paris-saclayupmc univ paris 06:sorbonne universites-f-91128 palaiseau cedexFrance cea damdifF-91297 ArpajonFrance cea saclay dsm/irfu/service d'astrophysiqueF-91191 Gif-sur-YvetteFrance institute of laser engineering osaka universitySuitaOsaka 565-0871Japan faculty of engineering sciences kyushu university6-1 Kasuga-KoenKasugaFukuoka 816-8580Japan luth observatoire de parispsl research universitycnrsuniversite paris diderotSorbonne Paris Cite92190 MeudonFrance universite de bordeaux-cnrs-cea celia UMR 5107F-33405 TalenceFrance gepi observatoire de parispsl research universitycnrsuniversite paris diderotSorbonne Paris Cite75014 ParisFrance graduate school of engineering osaka universitySuitaOsaka 565-0871Japan lerma observatoire de parispsl research universitycnrssorbonne universitesUPMC Univ.Paris 06F-75005 ParisFrance clarendon laboratory university of oxfordParks RoadOxford OX1 3PUUK flash center for computational science university of chicagoIL 60637USA

In this paper, we present a model characterizing the interaction of a radiative shock(RS) with a solid material, as described in a recent paper(Koenig et al., Phys. Plasmas, 24, 082707(2017)), the new model is then related to recent experiments performed on the gEKKO XII laser facility. The RS generated in a xenon gas cell propagates towards a solid obstacle that is ablated by radiation coming from the shock front and the radiative precursor, mimicking processes occurring in astrophysical phenomena. The model presented here calculates the dynamics of the obstacle expansion,which depends on several parameters, notably the geometry and the temperature of the shock. All parameters required for the model have been obtained from experiments. good agreement between experimental data and the model is found when spherical geometry is taken into account. As a consequence, this model is a useful and easy tool to infer parameters from experimental data(such as the shock temperature), and also to design future experiments.

关键词： high energy density physics laser–plasmas interaction modelling plasmas astrophysics plasma physics radiative hydrodynamics radiative shock

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Triggering star formation:Experimental compression of a foam ball induced by Taylor–Sedov blast waves

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Matter and Radiation at Extremes 2022年第3期7卷 31-39页

作者： B.Albertazzi P.Mabey Th.Michel g.rigon, J.R.Marques S.Pikuz S.Ryazantsev E.Falize L.Van Box Som J.Meinecke N.Ozaki g.gregori M.Koenig LULI-CNRS CEASorbonne UniversitesEcole PolytechniqueInstitut Polytechnique de ParisF-91120 Palaiseau cedexFrance Department of Physics Freie Universitat Berlin14195 BerlinGermany JIHT-RAS 13-2 Izhorskaya st.Moscow 125412Russia National Research Nuclear University“MEPhI ”Moscow 115409Russia CEA-DAM-DIF F-91297 ArpajonFrance Clarendon Laboratory University of OxfordParks RoadOxford OX13PUUnited Kingdom graduate School of Engineering Osaka UniversitySuitaOsaka 565-0871Japan Institute of Laser Engineering Osaka UniversitySuitaOsaka 565-0871Japan

The interaction between a molecular cloud and an external agent(e.g.,a supernova remnant,plasma jet,radiation,or another cloud)is a common phenomenon throughout the Universe and can significantly change the star formation rate within a *** process leads to fragmentation of the cloud and to its subsequent compression and can,eventually,initiate the gravitational collapse of a stable molecular *** is,however,difficult to study such systems in detail using conventional techniques(numerical simulations and astronomical observations),since complex interactions of flows *** this paper,we experimentally investigate the compression of a foam ball by Taylor–Sedov blast waves,as an analog of supernova remnants interacting with a molecular *** formation of a compression wave is observed in the foam ball,indicating the importance of such experiments for understanding how star formation is triggered by external agents.

关键词： cloud galaxy supernova

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On the study of hydrodynamic instabilities in the presence of background magnetic fields in high-energy-density plasmas

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Matter and Radiation at Extremes 2021年第2期6卷 37-45页

作者： M.J.-E.Manuel B.Khiar g.rigon B.Albertazzi S.R.Klein F.Kroll F.-E.Brack T.Michel P.Mabey S.Pikuz J.C.Williams M.Koenig A.Casner C.C.Kuranz general Atomics San DiegoCalifornia 92121USA University of Chicago ChicagoIllinois 60637USA Laboratoire pour l’utilisation des lasers intenses 91128 Palaiseau CedexFrance University of Michigan Ann ArborMichigan 48109USA Helmholtz-Zentrum Dresden-Rossendorf 01328 DresdenGermany Technische Universitat Dresden 01062 DresdenGermany National Research Nuclear University Moscow 115409Russia Centre lasers intenses et applications 33405 Talence CedexFrance

Blast-wave-driven hydrodynamic instabilities are studied in the presence of a background B-field through experiments and simulations in the high-energy-density(HED)physics *** experiments conducted at the Laboratoire pour l’utilisation des lasers intenses(LULI),a laserdriven shock-tube platform was used to generate a hydrodynamically unstable interface with a prescribed sinusoidal surface perturbation,and short-pulse x-ray radiography was used to characterize the instability growth with and without a 10-T *** LULI experiments were modeled in FLASH using resistive and ideal magnetohydrodynamics(MHD),and comparing the experiments and simulations suggests that the Spitzer model implemented in FLASH is necessary and sufficient for modeling these planar *** results suggest insufficient amplification of the seed B-field,due to resistive diffusion,to alter the hydrodynamic *** the ideal-MHD simulations did not represent the experiments accurately,they suggest that similar HED systems with dynamic plasma-β(=2μ_(0)ρv^(2)/B^(2))values of less than∼100 can reduce the growth of blast-wave-driven Rayleigh–Taylor *** findings validate the resistive-MHD FLASH modeling that is being used to design future experiments for studying B-field effects in HED plasmas.

关键词： field. hydrodynamic instabilities

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Laboratory radiative accretion shocks on gEKKO XⅡlaser facility for POLAR project

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High Power Laser Science and Engineering 2018年第2期6卷 181-188页

作者： L.Van Box Som E.Falize M.Koenig Y.Sakawa B.Albertazzi E Barroso J.-***-Bidaud C.Busschaert A.Ciardi Y.Hara N.Katsuki R.Kumar E Lefevre C.Michaut Th.Michel T.Miura T.Morita M.Mouchet g.rigon T.Sano S.Shiiba H.Shimogawara S.Tomiya CEA-DAM-DIF F-91297 ArpajonFrance LERMA Sorbonne UniversiteObservatoire de ParisUniversite PSLCNRSF-75005 ParisFrance CEA Saclay DSM/Irfu/Service d'AstrophysiqueF-91191 Gif-sur-YvetteFrance LULI-CNRS Ecole PolytechniqueCEA:Universite Paris-Saclay UPMC Univ Paris 06:Sorbonne Universite-F-91128 Palaiseau Cedex France graduate School of Engineering Osaka UniversitySuitaOsaka 565-0871Japan Institute of Laser Engineering Osaka UniversitySuitaOsaka 565-0871Japan Faculty of Engineering Sciences Kyushu University6-1 Kasuga-KoenKasugaFukuoka 816-8580Japan Aoyama gakuin University Japan gEPI Observatoire de ParisPSL Research UniversityCNRSUniversite Paris DiderotSorbonne Paris CiteF-75014 ParisFrance LUTH Observatoire de ParisPSL Research UniversityCNRSUniversite Paris DiderotSorbonne Paris CiteF-92195 MeudonFrance

A new target design is presented to model high-energy radiative accretion shocks in polars. In this paper, we present the experimental results obtained on the gEKKO XII laser facility for the POLAR project. The experimental results are compared with 2 D FCI2 simulations to characterize the dynamics and the structure of plasma flow before and after the collision. The good agreement between simulations and experimental data confirms the formation of a reverse shock where cooling losses start modifying the post-shock region. With the multi-material structure of the target,a hydrodynamic collimation is exhibited and a radiative structure coupled with the reverse shock is highlighted in both experimental data and simulations. The flexibility of the laser energy produced on gEKKO XII allowed us to produce high-velocity flows and study new and interesting radiation hydrodynamic regimes between those obtained on the LULI2000 and Orion laser facilities.

关键词： accretion processes high power laser hydrodynamics laboratory astrophysics

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Development of new diagnostics based on LiF detector for pump-probe experiments

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Matter and Radiation at Extremes 2018年第4期3卷 197-206页

作者： T.Pikuz A.Faenov NOzaki T.Matsuoka B.Albertazzi N.J.Hartley K.Miyanishi K.Katagiri S.Matsuyama K.Yamauchi H.Habara Y.Inubushi T.Togashi H.Yumoto H.Ohashi Y.Tange T.Yabuuchi M.Yabashi A.N.grum-grzhimailo A.Casner I.Skobelev S.Makarov S.Pikuz g.rigon M.Koenig K.A.Tanaka T.Ishikawa R.Kodama graduate School of Engineering Osaka UniversitySuitaOsaka 565-0871Japan Joint Institute for High Temperatures Russian Academy of SciencesMoscow 125412Russia Open and Transdisciplinary Research Initiatives Osaka UniversitySuitaOsaka 565-0871Japan Photon Pioneers Center Osaka UniversitySuitaOsaka 565-0871Japan LULI e CNRS Ecole PolytechniqueCEA:Universite Paris-SaclayUPMC Univ Paris 06:Sorbonne Universites-F-91128 Palaiseau cedexFrance Helmholtz-Zentrum Dresden-Rossendorf Dresden 01328Germany Japan Synchrotron Radiation Research Institute Sayo-choSayo-gunHyogo 679-5198Japan RIKEN Spring-8 Center Sayo-choSayo-gunHyogo 679-5148Japan Skobeltsyn Institute of Nuclear Physics Lomonosov Moscow State UniversityMoscow 119991Russia Universite de Bordeaux-CNRS-CEA CELIA(Center Lasers Intenses et Applications)UMR 5107F-33405 TalenceFrance National Research Nuclear University MEPhI Moscow 115409Russia ELI-NP/IFN-HH Maqurele-Bucharest 077125 Romania ILE Osaka UniversitySuitaOsaka 565-0871Japan

We present new diagnostics for use in optical laser pump-X-ray Free Electron Laser(XFEL)probe experiments to monitor dimensions,intensity profile and focusability of the XFEL beam and to control initial quality and homogeneity of targets to be driven by optical laser *** developing X-ray imaging,based on the use of an LiF crystal detector,we were able to measure the distribution of energy inside a hard X-ray beam with unprecedented high spatial resolution(~1 mm)and across a field of view larger than some *** diagnostic can be used in situ,provides a very high dynamic range,has an extremely limited cost,and is relatively easy to be implemented in pump-probe *** proposed methods were successfully applied in pump-probe experiments at the SPring-8 Angstrom Compact free electron LAser(SACLA)XFEL facility and its potential was demonstrated for current and future High Energy Density Science experiments.

关键词： XFEL Shock waves Pump-probe experiments High energy density science X-ray spectroscopy X-ray imaging

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Phase Contrast Micro-Computed Tomography of Biological Sample at SSRF

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Tsinghua Science and Technology 2010年第1期15卷 102-107页

作者：陈荣昌谢红兰 Luigi rigon 杜国浩 Edoardo Castelli 肖体乔 Shanghai Institute of Applied Physics Chinese Academy of Sciences Department of Physics University of Trieste INFN Sezione di Trieste

In line X-ray phase contrast micro-computed tomography （IL-XPCT）, which can be implemented at third generation synchrotron radiation sources or by using a micro-focus X-ray tube, is a powerful technique for non-destructive, high-resolution investigations of a broad variety of materials. At the Shanghai Synchrotron Radiation Facility （SSRF）, the X-ray Imaging and Biomedical Applications Beamline was built and started regular user operation in May 2009. Both qualitative （without phase retrieval） and quantitative （with phase retrieval） three-dimensional IL-XPCT experimental techniques have been established at the beamline IL-XPCT experiments of a test sample （plastic pipes） used to evaluate the technique, and of a biological sample （locust） at the beamline are reported. Two series of images, qualitative and quantitative, including tomographic slices and three-dimensional rendering images were obtained. In qualitative images, there is a strong edge-enhancement which leads to very clear sample contours, while in quantitative images, the edge-enhancement fades but quantitative measurement of sample＇s phase information could be achieved. The experiments demonstrate that the combination of qualitative and quantitative images is useful for biological sample studies.

关键词： X-ray phase contrast tomography phase retrieval synchrotron radiation

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In vivo tracking of tau pathology using positron emission tomography (PET) molecular imaging in small animals

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Translational Neurodegeneration 2014年第1期3卷 34-39页

作者： Eduardo rigon Zimmer Antoine Leuzy Venkat Bhat Serge gauthier Pedro Rosa-Neto Translational Neuroimaging Laboratory(TNL) McGill Center for Studies in AgingDouglas Mental Health University InstituteMcGill University6875 La Salle Blv-FBC room 3149MontrealQCH4H 1R3Canada Montreal Neurological Institute(MNI) MontrealCanada Department of Biochemistry Federal University of Rio Grande do Sul(UFRGS)Porto AlegreBrazil Department of Psychiatry McGill UniversityMontrealBrazil

Hyperphosphorylation of the tau protein leading to the formation of neurofibrillary tangles(NFTs)is a common feature in a wide range of neurodegenerative diseases known as tauopathies,which include Alzheimer’s disease(AD)and the frontotemporal dementias(FTDs).Although heavily investigated,the mechanisms underlying the pathogenesis and progression of tauopathies have yet to be fully *** this context,several rodent models have been developed that successfully recapitulate the behavioral and neurochemical features of tau pathology,aiming to achieve a better understanding of the link between tau and *** date,behavioral and biochemical parameters assessed using these models have been conducted using a combination of memory tasks and invasive methods such as cerebrospinal fluid(CSF)sampling or post-mortem ***,several novel positron emission tomography(PET)radiopharmaceuticals targeting tau tangles have been developed,allowing for non-invasive in vivo quantification of tau *** with tau transgenic models and micro-PET,these tracers hold the promise of advancing the development of theoretical models and advancing our understanding of the natural history of AD and non-AD *** this review,we briefly describe some of the most important insights for understanding the biological basis of tau pathology,and shed light on the opportunity for improved modeling of tau pathology using a combination of tau-radiopharmaceuticals and animal models.

关键词： Positron emission tomography Tau molecular agents Tau rodent models Tauopathies

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Bioelectrical impedance vector analysis evaluates cellularity and hydration in cirrhotic patients

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World Journal of Hepatology 2020年第12期12卷 1276-1288页

作者： Sabrina Alves Fernandes Lara rigon Leonhardt Daniella Miranda da Silva Fernanda Donner Alves Claudio Augusto Marroni Department of Nutrition Centro Universitario Metodista IPAPorto Alegre 90420-060RSBrazil gastroenterology and Hepatology Universidade Federal de Ciências da Saúde de Porto Alegre(UFCSPA)Porto Alegre 91760-470RSBrazil Postgraduate Program in Hepatology Universidade Federal de Ciências da Saúde de Porto Alegre(UFCSPA)Porto Alegre 90050-170RSBrazil Department of Nutrition Centro Universitario Ritter dos Reis-UniritterPorto Alegre 90840-440Rio Grande do SulBrazil

BACKgROUND Malnutrition in cirrhotic patients is correlated with mortality and a better response to liver ***,recovery of the nutritional status in these patients is a challenge due to the difficulty in establishing a reliable nutritional *** bioelectrical impedance vector analysis(BIVA)method appears as a feasible tool in clinical practice to define the physiological state of cirrhotic patients by assessing hydration and body *** To evaluate body composition in cirrhotic patients using *** This retrospective cross-sectional study was carried out by following cirrhotic outpatients at a hospital in Porto Alegre,Brazil.A tetrapolar bioelectrical impedance analysis device was used to evaluate cellularity and hydration and to perform the *** BIVA graphic was elaborated by software and for statistical analysis a significance level of 5%(P≤0.05)was *** One hundred and ninety patients,61.1%males,with a mean age of 56.6±11.0 years,were *** these,56.3%had Child-Turcotte-Pugh(CTP)A score,and the prevalent etiology was hepatitis C virus(47.4%).The patients were classified according to cellularity and hydration by the quadrants and ellipses of the BIVA method,quadrant 1(47.9%);quadrant 2(18.9%);quadrant 3(14.2%);and quadrant 4(18.9%).Those classified in quadrant 1 and 2 had a higher phase angle compared to those in quadrants 3 and 4(Pge age than the other *** association with CTP score showed that patients in quadrant 2 had a higher proportion of CTP A,and those in quadrant 4 had a higher proportion of CTP C(Pge and prognostic index.

关键词： Body composition Hydration Cellularity Hepatic cirrhosis Electrical Bioimpedance Bioelectrical impedance vector analysis

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Analysis of Morphological Processes in a Disturbed gravel-Bed River （Piave River）： Integration of LiDAR Data and Colour Bathymetry

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Journal of Civil Engineering and Architecture 2014年第5期8卷 639-648页

作者： Fabio Delai Johnny Moretto Lorenzo Picco Emanuel rigon Diego Ravazzolo Mario Aristide Lenzi Department of Land Environment Agriculture and Forestry University of Padova Legnaro 35020 Italy

The magnitude of river morphological changes are better analyzed through the use of quantitative approaches, wherein resolution accuracy and uncertainty assessment are treated as crucial key-factors. In this sense, the creation of precise DEMs （Digital Elevation Models） of rivers represents an affordable tool to analyze geomorphic variations and budgets, except for wetted areas, where reliable channel digitalization can normally be obtained only using expensive bathymetric surveys. The proposed work aims at improving channel surface models without having available bathymetric sensors, by deriving dry areas elevations from LiDAR data and water depth of wetted areas from aerial photos through a predictive depth-colour relationship. The methodology was applied to two different sub-reaches of the Piave River, a gravel-bed river which suffered severe flood events in 2010. Erosion and deposition patterns were identified through DEM differencing, showing a predominance of scour processes which can lead to channel instability situations. The bathymetric output was compared to other previously-derived models confirming the accuracy of the in-channel elevation estimates. Finally, a discussion on the role played by longitudinal protections during the studied flood events is proposed, focusing the attention on the incidence of two major bank erosions that removed significant volumes of stable areas.

关键词： Colour bathymetry LiDAR data flood impacts fluvial erosion-deposition processes effect of river protections.

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Turbulent hydrodynamics experiments in high energy density plasmas： scientific case and preliminary results of the TurboHEDP project

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High Power Laser Science and Engineering 2018年第3期6卷 50-64页

作者： A. Casner g. rigon B. Albertazzi Th. Michel T. Pikuz A. Faenov P. Mabey N. Ozaki Y. Sakawa T. Sano J. Ballet P. Tzeferacos D. Lamb E. Falize g. gregori M. Koenig Universite de Bordeaux-CNRS-CEA CELIA (CEntre Lasers Intenses et Applications) UMR 5107 F-33405 Talence France LULI- CNRS Ecole Polytechnique CEA Universite Paris-Saclay UPMC Univ Paris 06 : Sorbonne Universites -F-91128 Palaiseau cedex France ENS Lyon Universite de Lyon CHELS 69342 Lyon France Open and Transdisciplinary Research Initiatives Osaka University Suita Osaka 565-0871 Japan Joint Institute for High Temperature RAS Moscow 125412 Russia graduate School of Engineering Osaka University Suita Osaka 565-0871 Japan Institute of Laser Engineering Osaka University Suita Osaka 565-0871 Japan Laboratoire AIM CEA-IRFU/CNRS/Universite Paris Diderot Departement d'Astrophysique CEA Saclay F-91191 Gif sur Yvette France Flash Center for Computational Science University of Chicago USA CEA DAM DIF F-91297 Arpajon France Clarendon Laboratory University of Oxford Parks Road Oxford OX1 3PU UK

The physics of compressible turbulence in high energy density(HED) plasmas is an unchartered experimental *** of compressible and radiative flows relevant for astrophysics rely mainly on subscale parameters. Therefore,we plan to perform turbulent hydrodynamics experiments in HED plasmas(TurboHEDP) in order to improve our understanding of such important phenomena for interest in both communities: laser plasma physics and astrophysics. We will focus on the physics of supernovae remnants which are complex structures subject to fluid instabilities such as the Rayleigh–Taylor and Kelvin–Helmholtz instabilities. The advent of megajoule laser facilities, like the National Ignition Facility and the Laser Megajoule, creates novel opportunities in laboratory astrophysics, as it provides unique platforms to study turbulent mixing flows in HED plasmas. Indeed, the physics requires accelerating targets over larger distances and longer time periods than previously achieved. In a preparatory phase, scaling from experiments at lower laser energies is used to guarantee the performance of future MJ experiments. This subscale experiments allow us to develop experimental skills and numerical tools in this new field of research, and are stepping stones to achieve our objectives on larger laser facilities. We review first in this paper recent advances in high energy density experiments devoted to laboratory astrophysics. Then we describe the necessary steps forward to commission an experimental platform devoted to turbulent hydrodynamics on a megajoule laser facility. Recent novel experimental results acquired on LULI2000, as well as supporting radiative hydrodynamics simulations, are presented. Together with the development of LiF detectors as transformative X-ray diagnostics, these preliminary results are promising on the way to achieve micrometric spatial resolution in turbulent HED physics experiments in the near future.

关键词： high energy density physics inertial confinement fusion laboratory astrophysics plasmas astrophysics

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