arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2005.02424astro-ph.IMastro-ph.EP
收藏

The Search for MeV Electrons 2-45 AU from the Sun with the Alice Instrument Microchannel Plate Detector Aboard New Horizons

B. A. Keeney, M. Versteeg, J. Wm. Parker, S. A. Stern, P. Brunts, M. W. Davis, H. A. Elliott, K. Ennico, G. R. Gladstone, R. L. McNutt,, C. B. Olkin, K. D. Reth… 展开作者

B. A. Keeney, M. Versteeg, J. Wm. Parker, S. A. Stern, P. Brunts, M. W. Davis, H. A. Elliott, K. Ennico, G. R. Gladstone, R. L. McNutt,, C. B. Olkin, K. D. Retherford, K. N. Singer, J. R. Spencer, A. J. Steffl, H. A. Weaver, L. A. Young

英文摘要:

The Alice UV spectrograph aboard NASA's New Horizons mission is sensitive to MeV electrons that penetrate the instrument's thin aluminum housing and interact with its microchannel plate detector. We have searched for penetrating electrons at heliocentric distance of 2-45 AU, finding no evidence of discrete events outside of the Jovian magnetosphere. However, we do find a gradual long-term increase in the Alice instrument's global dark count rate at a rate of ~1.5% per year, which may be caused by a heightened gamma-ray background from aging of the spacecraft's radioisotope thermoelectric generator fuel. If this hypothesis is correct, then the Alice instrument's global dark count rate should flatten and then decrease over the next 5-10 years.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑