Manipulate
发表于 2025-3-21 17:54:21
书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0468162<br><br> <br><br>书目名称Instruments and Methods for the Radio Detection of High Energy Cosmic Rays读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0468162<br><br> <br><br>
受辱
发表于 2025-3-21 23:24:13
Radio Experiments for Air Shower Detection,limited electronics available at that time prevented to exploit the full potential of the radio detection method, and other methods, like the detection of fluorescence or Cherenkov light from air showers, have been more successful.
HEW
发表于 2025-3-22 00:52:33
A Reference Beacon for the Auger Engineering Radio Array,he radio pulse already in individual antennas. An event whose signal-to-noise ratio is so low that it could only be detected with interferometry will not be triggered. Thus, interferometry will not lower the detection threshold of AERA.
南极
发表于 2025-3-22 07:41:20
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cartilage
发表于 2025-3-22 09:27:05
Time Calibration of LOPES,us of this chapter is to explain by which methods a relative timing accuracy and precision of ~1 ns can be achieved. However, for pulse arrival time measurements at low signal-to-noise ratios, the uncertainty is dominated by noise and can be much larger than the calibration uncertainty, as it will be discussed in Chap. 6.
Capture
发表于 2025-3-22 14:27:47
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失望未来
发表于 2025-3-22 18:11:08
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crockery
发表于 2025-3-22 23:19:50
Conclusion,h other techniques. This thesis reflects the progress in the understanding of the radio emission and presents a set of methods which improved LOPES and will help to answer the open questions with AERA and LOFAR, the next generation digital radio arrays.
heartburn
发表于 2025-3-23 03:03:15
Book 2012 offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments..
减去
发表于 2025-3-23 07:30:34
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