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Uspekhi Fizicheskih Nauk, 1971
CONTENTS 1. Pulsed x-ray sources with field emission 61 2. Generators of high-power pulses of x-ray bremsstrahlung 64 3. Generation of x rays in pulsed discharges in air and other gases 66 4.
V A Tsukerman, L V Tarasova, S I Lobov
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CONTENTS 1. Pulsed x-ray sources with field emission 61 2. Generators of high-power pulses of x-ray bremsstrahlung 64 3. Generation of x rays in pulsed discharges in air and other gases 66 4.
V A Tsukerman, L V Tarasova, S I Lobov
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Microsystem Technologies, 1995
X-ray source based on Compton scattering of laser light on a tightly focused relativistic electron ...
F. Villa, A. Luccio, M. Zolotorev
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X-ray source based on Compton scattering of laser light on a tightly focused relativistic electron ...
F. Villa, A. Luccio, M. Zolotorev
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1982
X-rays are produced whenever electrons are suddenly brought to rest by colliding with matter. It is necessary therefore, for the following conditions to prevail: 1. a means of producing and sustaining a stream of electrons, i.e. a good vacuum, with a source of electrons which in most modern X-ray tubes is a heated filament; 2.
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X-rays are produced whenever electrons are suddenly brought to rest by colliding with matter. It is necessary therefore, for the following conditions to prevail: 1. a means of producing and sustaining a stream of electrons, i.e. a good vacuum, with a source of electrons which in most modern X-ray tubes is a heated filament; 2.
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AIP Conference Proceedings, 1994
Objects with temperatures on the order of 30 eV and luminosities around 1038 erg/s have been established as a separate class by the recent ROSAT observations. The prototype supersoft x‐ray source (SSS) is the well‐known x‐ray binary CAL83 in the LMC, which has an orbital period of 1.04d.
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Objects with temperatures on the order of 30 eV and luminosities around 1038 erg/s have been established as a separate class by the recent ROSAT observations. The prototype supersoft x‐ray source (SSS) is the well‐known x‐ray binary CAL83 in the LMC, which has an orbital period of 1.04d.
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X-Ray Spectrometry, 2009
Abstract In this work we report on the characterization of pulsed soft x‐rays emitted from laser‐produced plasma. The plasma was generated by a pulsed KrF excimer laser focused on pure Si, Cu and Ta targets by 40, 80 and 120 mJ laser energies.
SICILIANO, MARIA VITTORIA +3 more
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Abstract In this work we report on the characterization of pulsed soft x‐rays emitted from laser‐produced plasma. The plasma was generated by a pulsed KrF excimer laser focused on pure Si, Cu and Ta targets by 40, 80 and 120 mJ laser energies.
SICILIANO, MARIA VITTORIA +3 more
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Astronomische Nachrichten, 2010
AbstractThe workshop “Supersoft X‐ray Sources – New Developments” brought together observers and theoretician to discuss the present status and unsolved problems of supersoft source research. A large part of the workshop was devoted to optical novae and their supersoft state. Large samples of supersoft X‐ray sources were presented from nearby galaxies,
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AbstractThe workshop “Supersoft X‐ray Sources – New Developments” brought together observers and theoretician to discuss the present status and unsolved problems of supersoft source research. A large part of the workshop was devoted to optical novae and their supersoft state. Large samples of supersoft X‐ray sources were presented from nearby galaxies,
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2006
In this chapter, standard stationary-anode, rotating anode and microfocus X-ray tubes are described and the spectra from these tubes are compared with the output from synchrotron-radiation sources. The choice of beam size, X-ray wavelength, spectral composition, intensity, cross fire and beam stability are discussed and a description is given of the ...
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In this chapter, standard stationary-anode, rotating anode and microfocus X-ray tubes are described and the spectra from these tubes are compared with the output from synchrotron-radiation sources. The choice of beam size, X-ray wavelength, spectral composition, intensity, cross fire and beam stability are discussed and a description is given of the ...
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1992
The study of the X-ray emission from M31 is a young field, having its beginnings in the mid-1970’s. By 1991, however, a fairly good understanding of the various sources is at hand. The importance of these sources is the result of the happy fact that M31 is a normal, high-luminosity galaxy; it therefore provides a good opportunity to study the X-ray ...
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The study of the X-ray emission from M31 is a young field, having its beginnings in the mid-1970’s. By 1991, however, a fairly good understanding of the various sources is at hand. The importance of these sources is the result of the happy fact that M31 is a normal, high-luminosity galaxy; it therefore provides a good opportunity to study the X-ray ...
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2005
X-ray was the name given by W C Roentgen to the highly penetrating rays which emanated when high-energy lectrons struck a meta ltarget. On 8 November 1895, he noted for the first time this phenomenon and on 28 December 1895, he astonished the scientific world with his preliminary report "Ueber eine neue Artvon Strahlen" (along with experimental ...
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X-ray was the name given by W C Roentgen to the highly penetrating rays which emanated when high-energy lectrons struck a meta ltarget. On 8 November 1895, he noted for the first time this phenomenon and on 28 December 1895, he astonished the scientific world with his preliminary report "Ueber eine neue Artvon Strahlen" (along with experimental ...
openaire +3 more sources