Search results for "non-thermal"

showing 10 items of 33 documents

Landmarks in the historical development of twenty first century food processing technologies.

2017

International audience; Over a course of centuries, various food processing technologies have been explored and implemented to provide safe, fresher-tasting and nutritive food products. Among these technologies, application of emerging food processes (e.g., cold plasma, pressurized fluids, pulsed electric fields, ohmic heating, radiofrequency electric fields, ultrasonics and megasonics, high hydrostatic pressure, high pressure homogenization, hyperbaric storage, and negative pressure cavitation extraction) have attracted much attention in the past decades. This is because, compared to their conventional counterparts, novel food processes allow a significant reduction in the overall processi…

0106 biological sciencesEngineeringSociology of scientific knowledgeArchitectural engineeringEmerging food technologies[SDV.BIO]Life Sciences [q-bio]/BiotechnologyFood Handling[SDV]Life Sciences [q-bio]Hydrostatic pressureThermal processingNanotechnologyNovel food01 natural sciencesHistory 21st Century0404 agricultural biotechnologyHigh pressure homogenization010608 biotechnologyPressureHistorical review[SPI.GPROC]Engineering Sciences [physics]/Chemical and Process EngineeringUltrasonicsbusiness.industryTwenty-First CenturyTemperature04 agricultural and veterinary sciencesEnergy consumptionEquipment DesignFood safetyNon-thermal processing040401 food scienceFood processingbusinessConventional food process[SDV.AEN]Life Sciences [q-bio]/Food and NutritionFood ScienceFood research international (Ottawa, Ont.)
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Surface Micro Discharge–Cold Atmospheric Pressure Plasma Processing of Common House Cricket Acheta domesticus Powder: Antimicrobial Potential and Lip…

2021

The growing world population and the need to reduce the environmental impact of food production drive the exploration of novel protein sources. Insects are being cultivated, harvested, and processed to be applied in animal and human nutrition. The inherent microbial contamination of insect matrices requires risk management and decontamination strategies. Thermal sterilization results in unfavorable cooking effects and oxidation of fatty acids. The present study demonstrates the risk management in Acheta domesticus (home cricket) powder with a low-energy (8.7–22.0 mW/cm2, 5 min) semi-direct surface micro discharge (SMD)–cold atmospheric pressure plasma (CAPP). At a plasma power density lower…

0301 basic medicineHistologyAcheta domesticusBiomedical EngineeringBacillus cereusinsect powderBioengineeringAtmospheric-pressure plasmaBacillus subtilisMass spectrometrycold plasmaMicrobial decontaminationFood safetylipids03 medical and health sciences0404 agricultural biotechnologyHouse cricketFood scienceBacillus megaterium2. Zero hunger030109 nutrition & dieteticsbiologyChemistryfungimicrobial decontamination04 agricultural and veterinary sciencesSterilization (microbiology)biology.organism_classificationNon-thermal processing040401 food scienceLipids3. Good healthfood safety13. Climate actionAchetaCold plasmaInsect powderTP248.13-248.65BiotechnologyFrontiers in Bioengineering and Biotechnology
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Innovative non-thermal technologies affecting potato tuber and fried potato quality

2019

Abstract Background Potatoes are important tubers for human consumption, providing an essential source of energy and great nutritional characteristics for human health. However, before consumption, potato tubers need to be stored and processed. As frying is the most common technique used in potato processing, fried potato is the most important processed potato product. Some food characteristics, provided by the frying process, are considered desirable, but others are harmful to human health and, thereby the main challenge is to reduce the formation of the undesirable characteristics, without compromising the sensorial attributes. Scope and approach In this review, the origin, economic impor…

Acrylamide0303 health sciences030309 nutrition & dieteticsbusiness.industrymedia_common.quotation_subject04 agricultural and veterinary sciencesQuality040401 food sciencemergent technologiesBiotechnologyPotato processing03 medical and health sciencesHuman health0404 agricultural biotechnologyFryingEnvironmental scienceQuality (business)Potato tuberbusinessOil uptakeFried potatoesNon-thermal technologiesFood ScienceBiotechnologymedia_commonTrends in Food Science & Technology
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Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
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Dissipative Processes and Their Role in the Evolution of Radio Galaxies

2019

Particle acceleration in relativistic jets to very high energies occurs at the expense of the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that can trigger this dissipation is key to the characterization of the energy budgets and particle acceleration mechanisms at action in active galaxies. Instabilities and entrainment are two obvious candidates to trigger dissipation. On the one hand, supersonic, relativistic flows threaded by helical fields, as expected from the standard formation models of jets in supermassive black-holes, are unstable to a series of magnetohydrodynamical instabilities, such as the Kelvin-Helmholtz, current-driven, or possibly the p…

Active galactic nucleuslcsh:AstronomyRadio galaxyAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesKinetic energy01 natural scienceslcsh:QB1-991X-rays: binariesAstrophysical jet0103 physical sciencesrelativistic processes ISM: jets and outflows010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsMechanicsgalaxies: jetsradiation mechanisms: non-thermalDissipationAstrophysics - Astrophysics of GalaxiesParticle accelerationAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenamagnetohydrodynamicsGalaxies
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Application of pulsed electric fields in meat and fish processing industries: An overview.

2019

The market demand for new meat and fish products with enhanced physicochemical and nutritional properties attracted the interest of the food industry and academia to investigate innovative processing approaches such as pulsed electric fields (PEF). PEF is an emerging technology based on the application of electrical currents between two electrodes thus inducing electroporation phenomena and enabling a non-invasive modification of the tissues' structure. This review provides an overview of the current knowledge on the use of PEF processing in meat and fish to enhance the physicochemical and nutritional changes, as a preservation method, as well as for improving the extraction of high added-v…

AgingMeatFood industryChemical Phenomena030309 nutrition & dieteticsMeat Proteins03 medical and health sciences0404 agricultural biotechnologyFood QualityNon-thermal technologyAnimalsFood-Processing IndustryBy-products valorizationFish processing0303 health sciencesbusiness.industryFishes04 agricultural and veterinary sciencesFish products040401 food sciencePreservationMeat ProductsElectroporationSeafoodEnvironmental scienceFish <Actinopterygii>Food TechnologyDigestionBiochemical engineeringWater holdingbusinessTenderizationFood ScienceFood research international (Ottawa, Ont.)
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EVIDENCE OF NON-THERMAL X-RAY EMISSION FROM HH 80

2013

Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separate…

AstrofísicaCiencias AstronómicasCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIndividual: Iras 18162-2048 [Stars]//purl.org/becyt/ford/1 [https]Herbig-Haro objects ISM: jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: generalHigh Energy Physics - Phenomenology (hep-ph)Herbig-Haro objectsGeneral [X-Rays]jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: general [Herbig-Haro objects ISM]Jets And Outflows [Ism]ThermalProtostarstars: individualAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationX-rayAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]radiation mechanisms: non-thermalHerbig-Haro ObjectsAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Non-Thermal [Radiation Mechanisms]AstronomíaInterstellar mediumHigh Energy Physics - PhenomenologyISM: jets and outflowsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASThe Astrophysical Journal
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Multifrequency Studies of the Peculiar Quasar 4C +21.35 during the 2010 Flaring Activity

2014

著者人数: 290名

AstrofísicaelectronPhotontorusAstrophysics01 natural scienceslaw.inventiongalaxies: active – gamma rays: general – quasars: general – quasars: individual (4C +21.35) – radiation mechanisms: non-thermalactive gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermal [galaxies]lawblack hole: Kerrgalaxies: active; gamma rays: general; quasars: general; quasars: individual: 4C +21.35; radiation mechanisms: non-thermalopticalGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsenergy: highPhysicsphotonRadiusnon-thermal [radiation mechanisms]Synchrotrongamma ray: emissionactive [galaxies]astro-ph.COElectrónicaFísica nuclearElectricidadGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal; Nuclear and High Energy PhysicsAstrophysics - High Energy Astrophysical Phenomenaquasars: individual (4C +21.35)Astrophysics - Cosmology and Nongalactic AstrophysicsFlareradiation mechanisms: non-thermal; galaxies: active; quasars: general; quasars: individual (4C +21.35); gamma rays: observationsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAAstrophysics::High Energy Astrophysical Phenomenaeducationgalaxies: activeFOS: Physical sciencesquasars: individual: 4C +21.35Astrophysics::Cosmology and Extragalactic AstrophysicsVHEGLASTemission: modelTelescopeX-rayquasars: general0103 physical sciencessynchrotrongalaxies: active gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermalquasarflux: densityindividual: 4C +21.35 [quasars]Astrophysics::Galaxy AstrophysicsAstronomia Observacionsgeneral [quasars]010308 nuclear & particles physicsAstronomy and AstrophysicsQuasargamma rays: generalradiation mechanisms: non-thermalAstrophysics - Astrophysics of GalaxiesMAGICRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)ddc:520spectral[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [gamma rays]Fermi Gamma-ray Space Telescope
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Prompt TeV Emission from Cosmic Rays Accelerated by Gamma Ray Bursts Interacting with Surrounding Stellar Wind

2009

11 pages, 1 figure.--ISI article identifier:000263148600009.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0810.1287

Astrofísicaradiation mechanism: non-thermalMesongamma rays: burstsAstrophysics::High Energy Astrophysical PhenomenaNuclear Theorynon-thermal [radiation mechanism]FOS: Physical sciencesSynchrotron radiationCosmic rayAstrophysicsElectronAstrophysics::Cosmology and Extragalactic AstrophysicsStellar-wind bubbleAstrophysicsHigh Energy Physics - Phenomenology (hep-ph)NeutronNuclear ExperimentPhysicstheory [gamma rays]Astrophysics (astro-ph)Gamma raybursts [gamma rays]Astronomy and Astrophysicsgamma rays: theoryHigh Energy Physics - PhenomenologySpace and Planetary ScienceHigh Energy Physics::ExperimentGamma-ray burst
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The NHXM observatory

2011

Exploration of the X-ray sky has established X-ray astronomy as a fundamental astrophysical discipline. While our knowledge of the sky below 10 keV has increased dramatically (∼8 orders of magnitude) by use of grazing incidence optics, we still await a similar improvement above 10 keV, where to date only collimated instruments have been used. Also ripe for exploration is the field of X-ray polarimetry, an unused fundamental tool to understand the physics and morphology of X-ray sources. Here we present a novel mission, the New Hard X-ray Mission (NHXM) that brings together for the first time simultaneous high-sensitivity, hard-X-ray imaging, broadband spectroscopy and polarimetry. NHXM will…

Black-holesAcceleration mechanismCosmic Visionmedia_common.quotation_subjectPolarimetry7. Clean energy01 natural sciencesMissionsCosmologyPhysical cosmologyNon-thermal emissionAcceleration mechanism; Accretion physics; Black-holes; Compact objects; Cosmology; Missions; Non-thermal emission; X-ray imaging; X-ray polarimetry; Astronomy and Astrophysics; Space and Planetary ScienceObservatory0103 physical sciencesBroadbandX-ray polarimetry010303 astronomy & astrophysicsCompact objectsmedia_commonPhysics010308 nuclear & particles physicsX-ray imagingVegaAstronomyAstronomy and AstrophysicsAccretion physicsCosmologySkySpace and Planetary ScienceExperimental Astronomy
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