Search results for "Program"

showing 10 items of 5938 documents

Zvaigžņotā Debess: 2016/17, Ziema (234)

2016

Contents: “ZVAIGŽŅOTĀ DEBESS” FORTY YEARS AGO: A.Balklavs. New Possibilities in Search of Cosmic Gravitational Waves (abridged) ; E.Mūkins. «Venus-9» and «Venus-10» Scientific Accomplishment (abridged) ; DEVELOPMENTS in SCIENCE: K.Schwartz. The Unknown Solar Corona ; DISCOVERIES: I.Pundure. Gaia Has Obtained Billion-Star 3D Map ; SPACE RESEARCH and EXPLORATION: J.Jaunbergs. Tar Lakes of Titan ; R.Misa. A Step Closer to Stars ; CONFERENCES and MEETINGS: J.Balodis. Copernicus Is Becoming an Impressive Business ; K.Bērziņš. Conference of Young European Radioastronomers at the Latvian Centre in Germany ; FLASHBACK: A.Alksnis. Short Trips and Faraway Journeys (concluded) ; For SCHOOL YOUTH: D.Bo…

Astroloģija-pareģojumiESA Copernicus programmaLVU astronomijas studenti – vēstulesLatvijas 41.atklātā fizikas olimpiāde16.astronomijas amatieru salidojums Starspace observatorijā:NATURAL SCIENCES::Physics::Astronomy and astrophysics [Research Subject Categories]LU Astronomijas institūts 2015.gadāSaules aptumsumi filatēlijāMildai Zepei – 100“Zvaigžņotās Debess” autori – pasākums Latvijas Zinātņu akadēmijāMārtiņam Bucleram – 150Debess spīdekļi – 2016. gada rudensAstroloģija – astromaģijaEiropas jaunie radioastronomi latviešu centrā BonnāStarpzvaigžņu zonde StarChipZvaigžņu svītru fotogrāfijasSaules koronaGaia’s pirmais katalogs – miljardzvaigžņu 3D karteLatvijas līgums ar CERNValfrīdam Osvaldam – 100Titāns – darvas ezeriPilns Saules aptumsums Sulavesi salāSaules pulksteņi Latvijā 2011-2015Saules pulksteni Latvijas simtgadei
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The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

2021

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operati…

AstronomyLarge detector systems for particle and astroparticle physics; Optics; Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Real-time monitoringReal-time monitoring01 natural sciencesAugerSuccessful operationObservatoryopticalAPDshardwareAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsInstrumentationPhoton detectors for UVMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEEBCCDsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsAugerobservatoryRobotic telescopeG-APDsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSciences exactes et naturellesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesprogrammingdetector: fluorescencePhotometry (optics)0103 physical sciencesddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Physicsvisible and IR photons (solid-state) (PIN diodesCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingetc)fluorescence [detector]Pierre Auger Observatory010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsActive monitoringOpticsCCDslasermonitoringEMCCDsLarge detector systems for particle and astroparticle physicatmosphereExperimental High Energy PhysicsOpticEnvironmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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Discontinuous Gradient Constraints and the Infinity Laplacian

2012

Motivated by tug-of-war games and asymptotic analysis of certain variational problems, we consider a gradient constraint problem involving the infinity Laplace operator. We prove that this problem always has a solution that is unique if a certain regularity condition on the constraint is satisfied. If this regularity condition fails, then solutions obtained from game theory and $L^p$-approximation need not coincide.

Asymptotic analysisGeneral Mathematicsta111010102 general mathematicsMathematical analysisinfinity Laplace operator01 natural sciences010101 applied mathematicsConstraint (information theory)Mathematics - Analysis of PDEsOperator (computer programming)Infinity LaplacianFOS: Mathematics0101 mathematicsGame theorygradient constraint problemsAnalysis of PDEs (math.AP)MathematicsInternational Mathematics Research Notices
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Counseling and attention for the diversity: description of programs and actions in some emerging groups

2002

This article offers points for reflection, practical elements and criteria for adoption in relation to addressing diversity and its orientation. Formal and informal contexts are dealt with from a social and educational perspective; the diversity which can be found in the ordinary population and those included within the so called “emerging groups” are also focused on. Within this framework the function of the educational psychologist lies not only in knowing the basic characteristics of the groups which most represent diversity and in evaluating specific situations, but also in bringing solutions to the problems specific to each group, both as individuals and as a collective, by means of th…

Atención a la diversidad grupos emergentes orientación programas de intervención
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Report of the COSPAR Mars special regions colloquium

2010

International audience; In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > -25 degrees C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conser…

Atmospheric Science010504 meteorology & atmospheric sciencesPlanetary protectionLiquid waterAerospace EngineeringTerrainBACTERIAL-ACTIVITY01 natural sciencesSPACECRAFT SURFACESAstrobiologyWater-vaporSouth-pole snow0103 physical sciencesBacterial activitySpace research010303 astronomy & astrophysicsBacterial activity0105 earth and related environmental sciencesMartianCommittee on Space ResearchCOSPAR mars special regions colloquiumNear-surfaceAstronomy and AstrophysicsMars Exploration Program15. Life on landGround ice[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]GeophysicsLiquid water13. Climate actionSpace and Planetary ScienceGeneral Earth and Planetary SciencesHigh obliquitySea-iceUpper martian surfaceSpace-craft surfacesGeology
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The Arctic Cloud Puzzle: Using ACLOUD/PASCAL Multiplatform Observations to Unravel the Role of Clouds and Aerosol Particles in Arctic Amplification

2019

A consortium of polar scientists combined observational forces in a field campaign of unprecedented complexity to uncover the secrets of clouds and their role in Arctic amplification. Two research aircraft, an icebreaker research vessel, an ice-floe camp including an instrumented tethered balloon, and a permanent ground-based measurement station were employed in this endeavour. Clouds play an important role in Arctic amplification. This term represents the recently observed enhanced warming of the Arctic relative to the global increase of near-surface air temperature. However, there are still important knowledge gaps regarding the interplay between Arctic clouds and aerosol particles, surfa…

Atmospheric Science010504 meteorology & atmospheric sciencesbusiness.industryCloud computingPascal (programming language)010502 geochemistry & geophysics01 natural sciencesAerosolThe arcticEarth sciencesClimatologyddc:550Polar amplificationEnvironmental sciencebusinesscomputer0105 earth and related environmental sciencescomputer.programming_languageBulletin of the American Meteorological Society
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FIDO science payload simulating the Athena Payload

2002

[1] The Jet Propulsion Laboratory's Field Integrated Development and Operations rover (FIDO) emulates and tests operational rover capabilities for advanced Mars rover missions, such as those originally planned for the Mars Surveyor 2001 Rover and currently planned for the Athena Payload on the Mars Exploration Rovers scheduled for launch in 2003. This paper describes FIDO's science instrument payload, which is fully integrated with rover hardware and software. Remote science teams visualize instrument suite data and generate FIDO commands using the Web Interface for Telescience. FIDO's instrument suite has been used in terrestrial laboratory and field tests to simulate Mars operations, to t…

Atmospheric ScienceComputer scienceSoil ScienceAquatic ScienceOceanographyExploration of Marslaw.inventionSoftwareGeochemistry and PetrologylawEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyRemote sensingEcologySpectrometerbusiness.industryPaleontologyForestryMars Exploration ProgramRobot end effectorMars roverGeophysicsStereo imagingSpace and Planetary ScienceRadiancebusinessJournal of Geophysical Research: Planets
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Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

2010

Spirit Mars Rover Mission : Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryMars Exploration ProgramAquatic ScienceOceanographyExploration of MarsHavenAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Meteorites on Mars observed with the Mars Exploration Rovers

2008

[1] Reduced weathering rates due to the lack of liquid water and significantly greater typical surface ages should result in a higher density of meteorites on the surface of Mars compared to Earth. Several meteorites were identified among the rocks investigated during Opportunity's traverse across the sandy Meridiani plains. Heat Shield Rock is a IAB iron meteorite and has been officially recognized as “Meridiani Planum.” Barberton is olivine-rich and contains metallic Fe in the form of kamacite, suggesting a meteoritic origin. It is chemically most consistent with a mesosiderite silicate clast. Santa Catarina is a brecciated rock with a chemical and mineralogical composition similar to Bar…

Atmospheric ScienceEcologyPaleontologySoil ScienceForestryMars Exploration ProgramAquatic ScienceOceanographyIron meteoriteStrewn fieldAstrobiologyKamaciteMesosideriteGeophysicsImpact craterMeteoriteSpace and Planetary ScienceGeochemistry and PetrologyChondriteEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Evidence for montmorillonite or its compositional equivalent in Columbia Hills, Mars

2007

During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’’ encountered several similar samples that are distinctly different from Martian meteorites and known Gusev crater soils, rocks, and sediments. Occurring in a variety of contexts and locations, these ‘‘Independence class’’ samples are rough-textured, iron-poor (equivalent FeO 4 wt%), have high Al/Si ratios, and often contain unexpectedly high concentrations of one or more minor or trace elements (including Cr, Ni, Cu, Sr, and Y). Apart from accessory minerals, the major component common to these samples has a compositional profile of major and minor elements whic…

Atmospheric ScienceGeochemistryMarsSoil ScienceMineralogymontmorilloniteAquatic ScienceOceanographychemistry.chemical_compoundImpact craterGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)chemical compositionEarth-Surface ProcessesWater Science and TechnologyGusevMineralEcologyPaleontologyForestryColumbia HillsclayMars Exploration ProgramMars explorationSilicateGeophysicsMontmorilloniteMeteoritechemistrySpace and Planetary ScienceroverGusev CraterSoil horizonClay mineralsGeologyJournal of Geophysical Research
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