4 edition of Large-format high resolution microchannel plate detectors for ultraviolet astronomy found in the catalog.
Large-format high resolution microchannel plate detectors for ultraviolet astronomy
by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, D.C.], [Springfield, Va
Written in English
|Other titles||Large format high resolution microchannel ...|
|Series||[NASA contractor report] -- NASA CR-197993., NASA contractor report -- NASA CR-197993.|
|Contributions||United States. National Aeronautics and Space Administration.|
|The Physical Object|
Search the leading research in optics and photonics applied research from SPIE journals, conference proceedings and presentations, and eBooks. M.A. Gruntman, A.A. Kozochkina, and V.B. Leonas, Three large format microchannel plate stack for position-sensitive detector (design and performance characteristics), Report # (Preprint), 43 pages, Space Research Institute (IKI) of the USSR Academy of Sciences, Moscow,
It carried an imaging X-ray Telescope (XRT) with three focal plane instruments: two Position Sensitive Proportional Counters (PSPC), a High Resolution Imager (HRI), and a wide field camera (WFC) extreme ultraviolet telescope co-aligned with the XRT that covered the wave band between and 6 angstroms ( to keV). Purchase Advances in Electronics and Electron Physics, Volume 74 - 1st Edition. Print Book & E-Book. ISBN , Book Edition: 1.
Resolution vs. Count Rate Lawrence Livermore National Laboratory 0 5 10 15 20 25 30 35 40 Energy Resolution at eV Energy Resolution at eV Electronic Noise FWHM Resolution [eV] Output Count Rate [cps] No pile-up rejection was used. The Technology and Instrumentation in Particle Physics (TIPP ) conference is the second in the new series of international conferences in the field of particle physics sponsored by IUPAP. The program focuses on all areas of detector development and instrumentation in particle physics, astro-particle physics and closely related fields. Here is a rough general guideline: for the.
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Get this from a library. Large-format high resolution microchannel plate detectors for ultraviolet astronomy: final technical report.
[Christopher Martin; United States. National Aeronautics and. CONFERENCE PROCEEDINGS Papers Presentations Journals. Advanced Photonics Journal of Applied Remote SensingCited by: 9.
High Speed Large Format Photon Counting Microchannel Plate Imaging Sensors Oswald H. Siegmund, Camden Ertley, John V. Vallerga, for Astronomy and remote sensing. Detectors have been developed to cover a wide range of optical/UV sensing applications.
Formats of 25mm circular, and 50mm (Planacon) and mm square have been constructed, withFile Size: 8MB. Large area (20×20 cm 2) sealed tube detectors using novel borosilicate glass microchannel plates, with bialkali photocathodes and strip-line readouts are being developed for Cherenkov light s based on conventional sealed tubes with alumina brazed body construction and hot indium seals have been by: 1.
Introduction. In recent years we have implemented a variety of delay line image readout systems for high-resolution, large format, photon-counting microchannel plate (MCP) detectors in space instrumentation [1–3].The cross-strip (XS) anode concept (Fig. 1) [4,5] employs many of the physical design techniques used for the delay line anodes.
However, the XS anode works by charge division Cited by: Tremsin AS, Siegmund OHW, Vallerga JV, Hull JS () Novel high resolution readout for UV and X-ray photon counting detectors with microchannel plates. Proc SPIE – Google ScholarCited by: 9.
KEYWORDS: Electronics, Opacity, Sensors, Glasses, Ultraviolet radiation, Microchannel plates, Quantum efficiency, Atomic layer deposition, Spatial resolution, Neodymium Read Abstract + Microchannel plate sensors are widely used as photon counting imagers in many applications, including, astronomy, high energy physics, and remote sensing.
Development of Visible Light Sensitive Imaging Tubes with Microchannel Plate Intensifiers and Wedge and Strip Readout J. Vallerga, and S. Bowyer, “High efficiency photon counting detectors for the FAUST spacelab far ultraviolet astronomy payload”,IEEE trans “Investigation of large format microchannel plate Z configurations Cited by: 2.
Proc. SPIESpace Telescopes and Instrumentation Ultraviolet to Gamma Ray, (17 September ); doi: / HIGH-RESOLUTION DETECTORS FOR IMAGING AND SPECTROSCOPY AT ULTRAVIOLET AND SOFT X-RAY WAVELENGTHS J.G.
TIMOTHY, J.S. MORGAN and D.C. SLATER Center for Space Science and Astrophysics, Stanford University, ERLStanford, CAU.S.A. Abstract The presently performance-evaluated format, in which a high-gain curved-channel microchannel plate (M2MCP) has a spherical concave input face and a plane output face, allows the input face of the.
Large 20 cm square microchannel plate prototypes with 20 μm and 40 μm pores have been fabricated and initial tests show operational gain. Design and fabrication of a 20 cm sealed tube assembly is well advanced and comprises a borosilicate entrance window, a proximity focused bialkali photocathode, a pair of microchannel plates and a stripline Cited by: The high resolution photon/ion/electron/neutron counting capabilities of Microchannel Plate (MCP) detectors have been demonstrated previously with several readout technologies to timing resolution.
KEYWORDS: Spectrographs, Stars, Sensors, Microchannel plates, Quantum efficiency, Light scattering, Physics, Sensor performance, Atomic layer deposition, Extreme ultraviolet Read Abstract + We present the performance of a mm × mm microchannel plate detector during two suborbital flights in and Cloudy Nights Large Format The next step up is medium format " format rollfilm" and " format rollfilm".
The difference between the two is the length of the film - format gives you about 15 shots/roll when shot as There has been significant progress over the last few years in the development of technologies for microchannel plate (MCP) imaging detectors in the ultraviolet.
The nominal configuration of this type of detector consists of a photocathode to convert incoming radiation to photoelectrons, MCP’s to amplify the signals, followed by either an.
Development of Low-Temperature Detectors For Generation-X and Other Missions Requiring High-Resolution, Large-Format, X-ray Detector Arrays A White Paper submitted to Electromagnetic Observations from Space (EOS) Discipline Program Simon Bandler University of Maryland College Park & NASA / Goddard Space Flight Center () Simon.R.
detectors are a priority. Furthermore, these recommendations set as a goal very large format (i.e., Megapixel to Gigapixel), high quantum efficiency (QE), UV-sensitive detectors.
Additionally, the Association of Universities for Research in Astronomy (AURA), convened aCited by: Space Telescopes and Instrumentation Ultraviolet to Gamma Ray Editor(s): Monique Arnaud; Stephen S.
Murray ; Tadayuki Takahashi For the purchase of this volume in printed format, please visit High Energy, Optical, and Infrared Detectors for Astronomy VI Sunday - Wednesday 22 - 25 June.
The goal is to produce large-format, high QE, low-noise UV-sensitive detectors routinely that can be employed in a variety of explorer, medium, and strategic missions. Development of UV coatings with high reflectivity (>%), high uniformity .Chandra can detect x-ray photons with energy in the range ~ to 10 keV, with an effective area for imaging of cm 2 at ~1 keV; armed with charge-coupled devices (CCDs) and microchannel plate detectors, it has over a hundred times better sensitivity than the Einstein Observatory, which was launched inand 10 times the angular.Washington, DC: The National Academies Press.
doi: / (CCDs) and high-resolution, large-format anodes for improved microchannel plate detectors. None of these are likely to be challenging. The current baseline design of a segmented primary mirror might have low-enough scattered light to allow progress for observations of Earth.