Microchannel plates for the UVCS and SUMER instruments on the SOHO satellite
Microchannel plates for the UVCS and SUMER instruments on the SOHO satellite
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SOHO 卫星上 UVCS 和 SUMER 仪器的微通道板
DOI:
10.1117/12.218388
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发表时间:
1995
期刊:
影响因子:
--
通讯作者:
J. Vallerga
中科院分区:
文献类型:
--
作者:
O. Siegmund;M. Gummin;T. Sasseen;P. Jelinsky;G. Gaines;J. Hull;J. Stock;M. Edgar;B. Welsh;S. Jelinsky;J. Vallerga
The microchannel plates for the detectors in the SUMER and UVCS instruments aboard the Solar Orbiting Heliospheric Observatory (SOHO) mission to be launched in late 1995 are described. A low resistance Z stack of microchannel plates (MCPs) is employed in a detector format of 27 mm multiplied by 10 mm using a multilayer cross delay line anode (XDL) with 1024 by 360 digitized pixels. The MCP stacks provide gains of greater than 2 multiplied by 107 with good pulse height distributions (as low as 25% FWHM) under uniform flood illumination. Background rates of approximately equals 0.6 event cm-2 sec-1 are obtained for this configuration. Local counting rates up to approximately equals 800 events/pixel/sec have been achieved with little drop of the MCP gain. MCP preconditioning results are discussed, showing that some MCP stacks fail to have gain decreases when subjected to a high flux UV scrub. Also, although the bare MCP quantum efficiencies are close to those expected (approximately equals 10%), we found that the long wavelength response of KBr photocathodes could be substantially enhanced by the MCP scrubbing process. Flat field images are characterized by a low level of MCP fixed pattern noise and are stable. Preliminary calibration results for the instruments are shown.