Приклади вживання Synchrotron radiation Англійська мовою та їх переклад на Українською
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Cyclotron and synchrotron radiation.
Synchrotron radiation is highly polarized.
In a synchrotron, such radiation is called synchrotron radiation.
Synchrotron radiation is inherently polarised.
The visible light is emission from oxygen that has been heated by higher-energy(ultraviolet and X-ray) synchrotron radiation.
The Stanford Synchrotron Radiation Laboratory.
Only by accelerating electrons in a magnetic field can you get thecharacteristic radio emission that we have seen: synchrotron radiation.
That's synchrotron radiation from the Milky Way Galaxy.
Only acceleration of electrons in a magnetic field it is possible to obtain a characteristic radiation, which we saw the synchrotron radiation.
So we took it to the Stanford Synchrotron Radiation Laboratory in California, which is a particle accelerator.
When high-energy particles are in rapid motion,including electrons forced to travel in a curved path by a magnetic field, synchrotron radiation is produced.
This is called synchrotron radiation, and it's normally used to look at things like proteins and that sort of thing.
It is worth noting that working in SPring-8allows you to get unique data using synchrotron radiation- those that it are simply impossible to get somewhere else.
This is a light called synchrotron radiation, and it's formed from electrons spiraling around cosmic magnetic fields.
Shklovskii, when electrons and heavier charged particles traveling at velocities close to the velocity oflight are slowed down in a magnetic field(so-called synchrotron radiation).
Synchrotron radiation is also generated by astronomical objects, typically where relativistic electrons spiral(and hence change velocity) through magnetic fields.
Radio emission of this kind is generated in a process known as“Synchrotron Radiation”, in which electrons, moving at close to the speed of light, interact with powerful magnetic fields.
Synchrotron radiation beamlines are high-performance instruments that allow obtaining multi-scale and multi-task researches on materials of industrial as well as fundamental interest.
At such energies, electrons and positrons must be accelerated in a straight line; accelerating them in a ring would result inexcessive energy loss from a process called synchrotron radiation.
The delicate tendrils seen in visible light form whatastronomers call a“cage” around the rich tapestry of synchrotron radiation, which in turn encompasses the energetic fury of the X-ray disk and jets.
Synchrotron radiation may occur in accelerators either as a nuisance, causing undesired energy loss in particle physics contexts, or as a deliberately produced radiation source for numerous laboratory applications.
According to one put forward by earlier theoristsversions radionici able to generate so-called synchrotron radiation produced by accelerating charged particles under the influence of a magnetic field.
In the course of many years, the Applied Physics Department of YerPhI successfully investigates electron-energy structure ofnew wide-band laser materials using synchrotron radiation in various spectral regions.
We know that there mustbe a lot of high-energy electrons in the plane to produce the synchrotron radiation that we see, and we think they're produced by supernova remnants, but there don't seem to be enough.
In the sciences, the Academy funds projects on the geology, flora, and fauna of Israel, and facilitates the participation of Israeli scientists in research at international projects,such as high-energy physics at CERN and synchrotron radiation at the European Synchrotron Radiation Facility.
The properties of this radiation are such that it should be attributed to synchrotron radiation(magnetic bremsstrahlung)- the radiation of fast electrons in magnetic fields that are“frozen” into fluxes of stellar plasma ejected during the explosion of the supernova.
Lund is consistently ranked as the top university in Northern Europe in physical sciences and this excellence is now expanding through the building of two international research centres-MAX IV, a synchrotron radiation laboratory that opened in Lund in June 2016, and ESS, the European Spallation Source that is currently under construction and expected to be in operation in 2023.
In addition to relatively long-wavelength radiation, Jupiter also emits synchrotron radiation(also known as the Jovian decimetric radiation or DIM radiation) with frequencies in the range of 0.1- 15 GHz(wavelength from 3 m to 2 cm),[58] which is the bremsstrahlung radiation of the relativistic electrons trapped in the inner radiation belts of the planet.
Tasks: Catalytically active metal centers in biological proteins and synthetic model complexes will be characterized usingspectroscopic methods(in particular X-ray spectroscopy at synchrotron radiation sources) and theoretical approaches(density functional theory)Â In the frame of the Berlin Excellencecluster""Unicat"", to gain information on the molecular and electronic structures and their influence on the catalytic reactions.