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Spectral Slicing X-Ray Telescope

Optical Engineering, 1986
Layered synthetic microstructure (LSM) X-ray optics is investigated as a system for coupling a conventional glancing incidence X-ray mirror to a high sensitivity X-ray detector. It is shown that, by the use of figured LSM optics, it is possible to magnify the X-ray image produced by the primary mirrors so as to maintain their high inherent spatial ...
Richard B. Hoover   +2 more
openaire   +1 more source

X-ray Telescopes

1996
The spectra of stars, even for early-type (hot) stars, fall off steeply in the ultraviolet. The falloff is roughly according to the Wien radiation law that prevails on the short-wavelength side of the black-body radiation peak. Nevertheless, there has been considerable interest in the ultraviolet because many spectral features pertaining to ionized ...
openaire   +1 more source

Swift x-ray telescope (XRT)

SPIE Proceedings, 2003
The Swift Gamma-Ray Burst Explorer will be launched late in 2003 to make prompt multiwavelength observations of Gamma-Ray Bursts and Afterglows. The X-ray Telescope (XRT) provides key capabilities that permit Swift to determine GRB positions with several arcsecond accuracy within 100 seconds of the burst onset.
David N. Burrows   +8 more
openaire   +1 more source

New x-ray telescope design

SPIE Proceedings, 2003
The Solar X-ray Imager (SXI) is a complimentary, add-on instrument designed for use on the next generation of Geostationary Orbiting Environmental Satellites (GOES). Its primary mission is to continuously observe the full solar disc at X-ray wavelengths; including coronal holes, active regions, flares, and coronal mass ejections. For wide-field imaging
Atanassova, Martina, Harvey, James E.
openaire   +2 more sources

Hadamard X-ray Spectro-telescope

Advances in Space Research, 1982
Abstract The Hadamard X-ray Spectro-telescope consists of a flat Bragg crystal, an Hadamard mask and an imaging proportional counter. We have achieved α⧸▵α≈50, which is limited by the position resolution of the detector. This telescope is useful to observe the spectral structure of extended X-ray sources.
H. Tsunemi   +4 more
openaire   +1 more source

NeXT hard x-ray telescope

SPIE Proceedings, 2004
NeXT is Japan's 6th X-ray astronomical observatory following to ASTRO-E2. The launch is currently scheduled in 2010. One of the main goal of NeXT is to explore the hard X-ray Universe with newly developed hard X-ray telescope. The hard X-ray telescope utilizes multilayer-supermirror and high-throughput thin-foil optics technology.
Yasushi Ogasaka   +7 more
openaire   +1 more source

Observations of X-Ray Jets with the Yohkoh Soft X-Ray Telescope

Nippon Tenmon Gakkai obun kenkyu hokoku, 1992
Time series of Soft X-ray Telescope images have revealed many X-ray jets in the solar corona. The typical size of a jet is 5 × 103–4 × 105 km, the translational velocity is 30–300 km s−1, and the corresponding kinetic energy is estimated to be 1025 ...
K. Shibata   +14 more
semanticscholar   +1 more source

Goldhelox: A Soft X-Ray Solar Telescope

Journal of X-Ray Science and Technology, 1995
The Goldhelox Project is the construction and use of a near-normal incidence soft x-ray robotic solar telescope by undergraduate students at Brigham Young University. Once it is completed and tested, it will be deployed from a Get-Away-Special (GAS) canister in the bay of a space shuttle.
D S, Durfee   +13 more
openaire   +2 more sources

Equal-curvature grazing-incidence x-ray telescopes

Applied Optics, 2003
We introduce a new type of x-ray telescope design, an equal-curvature telescope. We simply add a second-order axial sag to the base grazing-incidence cone-cone telescope. The radius of curvature of the sag terms is the same on the primary surface and on the secondary surface.
Timo T, Saha, William, Zhang
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Orthogonal Mirror Telescopes for X-ray Astronomy

Applied Optics, 1971
Crossed mirror telescopes are presented as an alternative to the present telescope systems used in x-ray astronomy. These instruments generally have a higher x-ray collecting efficiency but a poorer angular resolution than the more conventional paraboloid-hyperboloid telescopes.
L P, Vanspeybroeck   +2 more
openaire   +2 more sources

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