Search results for "SCOPE"

showing 10 items of 2420 documents

Simbol-X Mirror Module Thermal Shields: II-Small Angle X-Ray Scattering Measurements

2009

The formation flight configuration of the Simbol-X mission implies that the X-ray mirror module will be open to Space on both ends. In order to reduce the power required to maintain the thermal stability and, therefore, the high angular resolution of the shell optics, a thin foil thermal shield will cover the mirror module. Different options are presently being studied for the foil material of these shields. We report results of an experimental investigation conducted to verify that the scattering of X-rays, by interaction with the thin foil material of the thermal shield, will not significantly affect the performances of the telescope.

PhysicsPhysics::Instrumentation and DetectorsScatteringbusiness.industryShieldsX-ray bursts X-ray imaging Lenses prisms and mirrorsParticle detectorlaw.inventionTelescopeSettore FIS/05 - Astronomia E AstrofisicaOpticslawShieldAngular resolutionSmall-angle scatteringbusinessX- and gamma-ray telescopes and instrumentation X-ray scattering X-ray sourceFOIL methodAIP Conference Proceedings
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A Very Large Area Telescope for γ-Ray Astronomy Above 100 MeV Employing Limited Streamer Tubes

1994

A new detector for γ-ray astronomy above 100 MeV is described in which the electron-positron pairs are tracked by means of a set of plane arrays of Limited Streamer Tubes. This technique allows to build up very large area experiments which are specifically useful to study variable or transient sources.

PhysicsPhysics::Instrumentation and Detectorsbusiness.industryPlane (geometry)DetectorAstronomyGamma-ray astronomylaw.inventionTelescopePrimary mirrorOpticsObservational astronomylawTransient (oscillation)business
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FRAM—The Robotic Telescope for the Monitoring of the Wavelength Dependence of the Extinction: Description of Hardware, Data Analysis, and Results

2010

FRAM-F/(Ph)otometric Robotic Atmospheric Monitor is one of the atmospheric monitoring instruments at the Pierre Auger Observatory in Argentina. FRAM is an optical telescope equipped with CCD cameras and photometer, and it automatically observes a set of selected standard stars. Primarily, FRAM observations are used to obtain the wavelength dependence of the light extinction. FRAM telescope is also able to observe secondary astronomical targets, and namely the detection of optical counterparts of gamma-ray bursts has already proven to be successful. Finally, a wide-field CCD camera of FRAM can be used for rapid monitoring of atmospheric conditions along the track of particularly interesting …

PhysicsPierre Auger ObservatoryArticle Subjectbusiness.industrylcsh:AstronomyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsCosmic rayPhotometerOptical telescopelaw.inventionTelescopelcsh:QB1-991StarsOpticsRobotic telescopeSpace and Planetary SciencelawExtinction (optical mineralogy)Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsbusinessComputer hardwareRemote sensingAdvances in Astronomy
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Xrase: The X-Ray Spectroscopic Explorer

2001

The X-Ray Spectroscopic Explorer (XRASE) has a unique combination of features that will make it possible to address many of NASA’s scientific goals. These include how galaxy clusters form, the physics and chemistry of the ISM, the heating of stellar coronae, the amount and content of intergalactic baryonic matter, the mass of black holes and the formation of disks and jets in AGN and galactic binaries. XRASE has a thin foil, multilayered telescope with a large collecting area up to 10 keV, especially in the Fe Kα region (1100 cm2). Its microcalorimeter array combines high energy resolution (7 eV at 6 keV) and efficiency with a field-of-view of 26 arcmin2. A deep orbit allows for long, conti…

PhysicsPoint spread functionAstrophysics::High Energy Astrophysical PhenomenaX-rayAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicslaw.inventionTelescopeBaryonOrbitlawIntergalactic travelTransition edge sensorAstrophysics::Galaxy AstrophysicsGalaxy cluster
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Panel Discussion on Data Analysis Trends in X-Ray and γ-Ray Astronomy 30/5/84, 11°°–12°°

1985

[The text of the panel has been edited by Dr. ozel (with indispensable help from Gabi Breuer, secretary of MPIfR) from a tape recording. The words not completely understandable are noted by (?), while various inclusions for the continuity of the text are indicated by [ ]. The slides and viewgraphs presented in the panel are added as Figures and Tables.]

PhysicsPoint spread functionCompton telescopeX-rayCompton scatteringAstronomyAstrophysicsPattern recognition problemPanel discussion
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Quasi-isotropic 3-D resolution in two-photon scanning microscopy.

2009

One of the main challenges in three-dimensional microscopy is to overcome the lack of isotropy of the spatial resolution, which results from the axially-elongated shape of the point spread function. Such anisotropy gives rise to images in which significant axially-oriented structures of the sample are not resolved. In this paper we achieve an important improvement in z resolution in two-photon excitation microscopy through spatial modulation of the incident beam. Specifically, we demonstrate that the design and implementation of a simple shaded ring performs quasi-isotropic three-dimensional imaging and that the corresponding loss in luminosity can be easily compensated by most available fe…

PhysicsPoint spread functionbusiness.industryIsotropyResolution (electron density)Physics::OpticsAtomic and Molecular Physics and OpticsOpticsTwo-photon excitation microscopyMicroscopyFemtosecondNear-field scanning optical microscopebusinessImage resolutionOptics express
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Reduction of focus size in tightly focused linearly polarized beams

2004

The electromagnetic theory predicts that when a linearly polarized collimated field is focused by a high-angle focusing system, components perpendicular to the initial polarization are generated. The use of annular masks to reduce the area of the focal spot usually increases the magnitude of this phenomenon, known as depolarization. We present a class of masks, the three-ring masks, which are important because they narrow the central lobe of the focal intensity distribution without increasing the depolarization. This can be very useful in modern optical applications, such as confocal microscopy or multiphoton scanning microscopy.

PhysicsPolarized light microscopyPhysics and Astronomy (miscellaneous)Linear polarizationbusiness.industryDepolarizationPolarization (waves)Collimated lightlaw.inventionOpticsOptical microscopelawConfocal microscopyPerpendicularbusinessApplied Physics Letters
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Control of the speed of a DC motor by employeeing pulse width modulation (PWM) technique

2009

This paper is mainly focused on the technique of pulse width modulation for controlling the speed of a 12 volt DC motor more efficiently. A potentiometer was used to generate a wide variety of pulses. The output of the controlling circuit (Pulse Width) was connected to the second circuit as input for direction control. Here a single push switch was used to change the state (stopforward-stop-reverse) of the DC motor. These two circuits were combined into one for ease of use. Third circuit was designed to measure the speed of the motor by employing an opto-electronic sensor, an amplifier and a two blade fan to interrupt the signal transmission of the sensor. Finally, the output of the sensor …

PhysicsPulse-frequency modulationbusiness.industryDuty cyclePush switchAmplifierElectrical engineeringPotentiometerOscilloscopebusinessDC motorPulse-width modulation2009 12th International Conference on Computers and Information Technology
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The Joint SLR (Optical Range) and Radar-VLBI Satellite Observations using VIRAC Radio Telescope RT32, RT16 and SLR Station Riga

2020

Abstract Joint VLBI and SLR satellite tracking is a novel tracking approach to explore potential applications and to work out common procedures to coordinate observations between astronomical observatories in Latvia. Global Navigation Satellite System (GNSS) satellites equipped with laser retroreflectors have been chosen as test targets because they are accessible by both measuring techniques – satellite laser ranging (SLR) and Very Long Base Interferometry (VLBI). The first Joint SLR and VLBI observations of selected GNSS satellites using three of Latvian large-scale astronomical utilities – VIRAC radio telescopes RT32 and RT16 (Ventspils International Radio Astronomy Centre of Ventspils U…

PhysicsQC1-999General EngineeringGeneral Physics and Astronomylaw.inventionvlbiRadio telescopejoint observationslawgnss satellitesslrVery-long-baseline interferometryRange (statistics)SatelliteRadarJoint (geology)GeologyRemote sensingLatvian Journal of Physics and Technical Sciences
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Maximizing the information gain of a single ion microscope using bayes experimental design

2016

We show nanoscopic transmission microscopy, using a deterministic single particle source and compare the resulting images in terms of signal-to-noise ratio, with those of conventional Poissonian sources. Our source is realized by deterministic extraction of laser-cooled calcium ions from a Paul trap. Gating by the extraction event allows for the suppression of detector dark counts by six orders of magnitude. Using the Bayes experimental design method, the deterministic characteristics of this source are harnessed to maximize information gain, when imaging structures with a parametrizable transmission function. We demonstrate such optimized imaging by determining parameter values of one and …

PhysicsQuantum PhysicsMicroscopeDetectorFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural scienceslaw.inventionBayes' theoremSignal-to-noise ratioOrders of magnitude (time)law0103 physical sciencesMicroscopyIon trapQuantum Physics (quant-ph)010306 general physics0210 nano-technologyBiological systemNanoscopic scaleSPIE Proceedings
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