Influence of the microchannel plate and anode gap parameters on the spatial resolution of an image intensifier

Author(s):  
T. H. Hoenderken ◽  
C. W. Hagen ◽  
J. E. Barth ◽  
P. Kruit ◽  
G. O. Nützel
1986 ◽  
Author(s):  
George J. Yates ◽  
Steven A. Jaramillo ◽  
Paul Zagarino ◽  
Matt Thomas

2019 ◽  
Vol 14 (0) ◽  
pp. 1402128-1402128
Author(s):  
Canbin HUANG ◽  
Kazuaki HANADA ◽  
Kengoh KURODA ◽  
Shinichro KOJIMA ◽  
Hiroaki FUJIYOSHI ◽  
...  

2007 ◽  
Vol 25 (2) ◽  
pp. 519-532 ◽  
Author(s):  
N. P. Bannister ◽  
E. J. Bunce ◽  
S. W. H. Cowley ◽  
R. Fairbend ◽  
G. W. Fraser ◽  
...  

Abstract. A comprehensive understanding of the solar wind interaction with Earth's coupled magnetosphere-ionosphere system requires an ability to observe the charged particle environment and auroral activity from the same platform, generating particle and photon image data which are matched in time and location. While unambiguous identification of the particles giving rise to the aurora requires a Low Earth Orbit satellite, obtaining adequate spatial coverage of aurorae with the relatively limited field of view of current space bourne auroral imaging systems requires much higher orbits. A goal for future satellite missions, therefore, is the development of compact, wide field-of-view optics permitting high spatial and temporal resolution ultraviolet imaging of the aurora from small spacecraft in low polar orbit. Microchannel plate optics offer a method of achieving the required performance. We describe a new, compact instrument design which can observe a wide field-of-view with the required spatial resolution. We report the focusing of 121.6 nm radiation using a spherically-slumped, square-pore microchannel plate with a focal length of 32 mm and an F number of 0.7. Measurements are compared with detailed ray-trace simulations of imaging performance. The angular resolution is 2.7±0.2° for the prototype, corresponding to a footprint ~33 km in diameter for an aurora altitude of 110 km and a spacecraft altitude of 800 km. In preliminary analysis, a more recent optic has demonstrated a full width at half maximum of 5.0±0.3 arcminutes, corresponding to a footprint of ~1 km from the same spacecraft altitude. We further report the imaging properties of a convex microchannel plate detector with planar resistive anode readout; this detector, whose active surface has a radius of curvature of only 100 mm, is shown to meet the spatial resolution and sensitivity requirements of the new wide field auroral imager (WFAI).


Author(s):  
Klaus Heinemann ◽  
Helmut Poppa

The efficiency of electron microscope image intensification (EMII) systems is often represented in terms of signal-to-noise ratio as a function of current density in the final microscope image plane. Such a characteristic is one way of evaluating the sensitivity of an EMII-system. It determines the intensification necessary to raise the signals of individual electrons well above the equipment noise level of the intensifier/display chain.This approach to the problem of EMU may lead to misinterpretations since it does not consider the spatial resolution in the specimen. Usually, the spatial resolution of the EMII-chain is considerably inferior to the resolution of conventional photographic material. In internal photography one can, therefore, normally work with considerably lower electron optical magnifications than with an image intensifier system to resolve specimen details of the same dimensions.


2017 ◽  
Vol 46 (10) ◽  
pp. 1003005 ◽  
Author(s):  
谢运涛 Xie Yuntao ◽  
张玉钧 Zhang Yujun ◽  
王 玺 Wang Xi ◽  
孙晓泉 Sun Xiaoquan

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