• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利:CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验

假设SETI微波观测系统在星系中运行,用该系统对地球进行探测。

Detection of the Earth with the SETI microwave observing system assumed to be operating out in the galaxy.

作者信息

Billingham J, Tarter J

机构信息

NASA Ames Research Center, Moffett Field, CA 94035, USA.

出版信息

Acta Astronaut. 1992 Mar-Apr;26(3-4):185-8. doi: 10.1016/0094-5765(92)90093-x.

DOI:10.1016/0094-5765(92)90093-x
PMID:11537161
Abstract

This paper estimates the maximum range at which radar signals from the Earth could be detected by a search system similar to the NASA Search for Extraterrestrial Intelligence Microwave Observing Project (SETI MOP) assumed to be operating out in the galaxy. Figures are calculated for the Targeted Search, and for the Sky Survey parts of the MOP, both operating, as currently planned, in the second half of the decade of the 1990s. Only the most powerful terrestrial transmitters are considered, namely, the planetary radar at Arecibo in Puerto Rico, and the ballistic missile early warning systems (BMEWS). In each case the probabilities of detection over the life of the MOP are also calculated. The calculation assumes that we are only in the eavesdropping mode. Transmissions intended to be detected by SETI systems are likely to be much stronger and would of course be found with higher probability to a greater range. Also, it is assumed that the transmitting civilization is at the same level of technological evolution as ours on Earth. This is very improbable. If we were to detect another technological civilization, it would, on statistical grounds, be much older than we are and might well have much more powerful transmitters. Both factors would make detection by the NASA MOP a much more likely outcome.

摘要

本文估算了一个类似于美国国家航空航天局地外文明搜索微波观测项目(SETI MOP)的搜索系统在银河系中运行时,能够探测到来自地球的雷达信号的最大距离。计算了在20世纪90年代后半期按当前计划运行的定向搜索以及MOP的巡天部分的相关数据。仅考虑了地球上最强大的发射源,即位于波多黎各阿雷西博的行星雷达以及弹道导弹预警系统(BMEWS)。在每种情况下,还计算了MOP运行期间的探测概率。该计算假设我们仅处于窃听模式。旨在被SETI系统探测到的传输信号可能要强得多,当然在更大范围内被发现的概率也会更高。此外,假设发射文明的技术发展水平与地球上的我们处于同一水平。这是极不可能的。如果我们要探测到另一个技术文明,从统计学角度来看,它很可能比我们古老得多,而且很可能拥有强大得多的发射源。这两个因素都会使美国国家航空航天局的MOP更有可能探测到信号。

相似文献

1
Detection of the Earth with the SETI microwave observing system assumed to be operating out in the galaxy.假设SETI微波观测系统在星系中运行,用该系统对地球进行探测。
Acta Astronaut. 1992 Mar-Apr;26(3-4):185-8. doi: 10.1016/0094-5765(92)90093-x.
2
Risk and value analysis of SETI.搜寻地外文明计划(SETI)的风险与价值分析
Acta Astronaut. 1990;21(2):69-72. doi: 10.1016/0094-5765(90)90128-8.
3
Status of the NASA SETI Sky Survey microwave observing project.美国国家航空航天局搜寻地外文明计划天空调查微波观测项目的现状。
Acta Astronaut. 1992 Mar-Apr;26(3-4):177-84. doi: 10.1016/0094-5765(92)90092-w.
4
An assessment of the impact of radiofrequency interference on microwave SETI searches.射频干扰对微波地外文明搜索影响的评估。
Acta Astronaut. 1992 Mar-Apr;26(3-4):227-32. doi: 10.1016/0094-5765(92)90102-o.
5
The windows of SETI--frequency and time in the search for extraterrestrial intelligence.搜寻地外文明计划的窗口——寻找外星智慧中的频率与时间
Planet Rep. 1987 Nov-Dec;7(6):23-5.
6
A reply from Earth?来自地球的回复?
Acta Astronaut. 1992 Mar-Apr;26(3-4):295-7. doi: 10.1016/0094-5765(92)90115-y.
7
SETI target selection.搜寻地外文明计划目标选择。
Acta Astronaut. 1995 May-Jun;35(9-11):741-4. doi: 10.1016/0094-5765(95)00028-x.
8
A search for narrow band signals with SERENDIP II: a progress report.
Acta Astronaut. 1988;17(1):123-7. doi: 10.1016/0094-5765(88)90135-x.
9
Ultranarrowband searches for extraterrestrial intelligence with dedicated signal-processing hardware.使用专用信号处理硬件进行超窄带地外文明搜索。
Icarus. 1986;67:525-39. doi: 10.1016/0019-1035(86)90129-6.
10
Radio frequency interference at Jodrell Bank Observatory within the protected 21 cm band.焦德雷尔班克天文台在受保护的21厘米波段内的射频干扰。
Acta Astronaut. 1989;19(11):907-12. doi: 10.1016/0094-5765(89)90083-0.