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Showing 1 to 13 of 13 for “"X-ray Telescope"”.

  1. Preflare observations using the Skylab X-ray telescope

    Thesis. 1977. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.

    mit Repository record for Preflare observations using the Skylab X-ray telescope (opens in a new tab)

  2. X-ray telescope foil optics : assembly, metrology, and constraint

    Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Mechanical Engineering, 2003.

    mit Repository record for X-ray telescope foil optics : assembly, metrology, and constraint (opens in a new tab)

  3. Ion implantation for figure correction of high-resolution x-ray telescope mirrors

    … for future high-resolution, large-aperture x-ray telescopes continues to challenge the x-ray astronomy instrumentation community. Building a large-aperture telescope requires thin, lightweight mirrors; due to the very low stiffness of thin mirrors, these are difficult to fabricate, coat, and …

    mit Repository record for Ion implantation for figure correction of high-resolution x-ray telescope mirrors (opens in a new tab)

  4. Design and modeling of a third generation slumping tool for X-ray telescope mirrors/

    … 5 arcsec are in demand for the International X-Ray Observatory. Several glass flattening techniques are presented in this thesis, including a method of thermally shaping individual sheets of glass using porous mandrels as air bearings developed at the Space Nanotechnology Lab. This method, a …

    mit Repository record for Design and modeling of a third generation slumping tool for X-ray telescope mirrors/ (opens in a new tab)

  5. Microcomb fabrication for high accuracy foil x-ray telescope assembly and vector Gaussian beam modeling

    Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Electrical Engineering and Computer Science, 2000.

    mit Repository record for Microcomb fabrication for high accuracy foil x-ray telescope assembly and vector Gaussian beam modeling (opens in a new tab)

  6. The Design and Analysis of Several Configurations for a Two Channel, Three Mirror X-Ray Telescope.

    In 1922, Compton [2] first reported reflecting x-rays from polished surfaces of glass and other materials. The angles of incidence required were very large—in the case of glass, 89 degrees 49 minutes of arc—for reflection of x-rays of 1.27Ã… wavelength. Such reflection of x-rays is called …

    uab Repository record for The Design and Analysis of Several Configurations for a Two Channel, Three Mirror X-Ray Telescope. (opens in a new tab)

  7. Metrology and mechanics for manufacturing space-based x-ray grating spectrometers

    … optical systems in many fields - including telescope, microscopy, lithography, and display technologies. A space x-ray telescope needs more stringent requirements as it observes distant space objects using a limited number of x-ray photons in a harsh space environment. The optical …

    mit Repository record for Metrology and mechanics for manufacturing space-based x-ray grating spectrometers (opens in a new tab)

  8. Imaging X-ray spectroscopy with micro-X and Chandra

    High spectral resolution observations of X-ray phenomena have the potential to uncover new physics. Currently, only point sources can be probed with high resolution spectra, using gratings. Extended objects like supernova remnants cannot be dispersed, leaving the dense forest of emission lines …

    mit Repository record for Imaging X-ray spectroscopy with micro-X and Chandra (opens in a new tab)

  9. High-resolution studies of charge exchange in supernova remnants with Magellan, XMM-Newton, and Micro-X

    … in two energy bands: the optical and the X-ray. The optical study, performed using both imaging and high resolution spectroscopy from the IMACS instrument on the Magellan Baade Telescope at Las Campanas Observatory, seeks to identify 'Balmer-dominated shocks' in the remnant, which signal the …

    mit Repository record for High-resolution studies of charge exchange in supernova remnants with Magellan, XMM-Newton, and Micro-X (opens in a new tab)

  10. EUV Spectroscopy of Solar Active Region Jets

    … imaging observations from space-based telescopes such as the Atmospheric Imaging Assembly (AIA) instrument on board the Solar Dynamic Observatory (SDO), the X-ray Telescope (XRT) on board the Hinode satellite, and spectroscopic observations from the Extreme UV Imaging Spectrometer (EIS) …

    cambridge Repository record for EUV Spectroscopy of Solar Active Region Jets (opens in a new tab)

  11. Methods of improving the surface flatness of thin glass sheets and silicon wafers

    … disk drive industry for making platters, the x-ray telescope industry for making high precision optics, and the semiconductor industry for making masks and substrates. The exceptional optical qualities of sheet glass give them a leading advantage in many technologies; however, one main …

    mit Repository record for Methods of improving the surface flatness of thin glass sheets and silicon wafers (opens in a new tab)

  12. Accretion flows and neutron star heating in low-mass X-ray binaries

    X-ray binaries are excellent test beds for studies of high-energy accretion flows and the properties of compact objects. Neutron star (NS) low-mass X-ray binaries (LMXBs) vary in brightness by almost 8 orders of magnitude and are hosts to diverse accretion flows, transporting varying amounts of …

    mit Repository record for Accretion flows and neutron star heating in low-mass X-ray binaries (opens in a new tab)

  13. Optimizing The Performance Of As-manufactured Grazing Incidence X-ray Telescopes Using Mosaic Detector Arrays

    The field of X-ray astronomy is only forty (43) years old, and grazing incidence X-ray telescopes have only been conceived and designed for a little over fifty (50) years. The Wolter Type I design is particularly well suited for stellar astronomical telescopes (very small field-of-view). The first …

    ucf