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

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.     

The SERENDIP SETI project: new instrumentation for SETI and results of recent observations

Over the past 30 years research into the existence of extraterrestrial life has focused on attempts to detect stable narrowband radio signals emitted in the microwave portion of the radio frequency (RF) spectrum. The SERENDIP SETI group is currently conducting search operations on the world’s largest radio telescope at the Arecibo Observatory in Puerto Rico.The third generation SERENDIP system, SERENDIP III, is a 4 million channel FFT-based spectrum analyzer with 0.6 Hz frequency resolution. In this paper, we will discuss the results of our recent 3.5 year sky survey. SERENDIP looked at 95% of the sky visible from Arecibo in the 424–436 MHz range, analyzed 10¹⁴ spectral bins, and logged information on over 2.5×10⁸ signals.The fourth generation SERENDIP system expands on the SERENDIP III design. SERENDIP IV computes 2×10¹¹ operations each second, providing spectral analysis on 160 million channels in 1.7 s. We will discuss the design and use of the SERENDIP IV system and future observing plans.     

An assessment of the impact of radiofrequency interference on microwave SETI searches

Investigations are carried out at JPL on radiofrequency interferences at very low levels (-130 to -180 dBm) in various bands, especially the 1-2 GHz band. Extrapolation of interferences in the years to come is attempted.     

Status of CHIPS: A NASA university explorer astronomy mission

In the age of `Faster, Better, Cheaper', NASA's Goddard Space Flight Center has been looking for a way to implement university based world class science missions for significantly less money. The University Explorer (UNEX) program is the result. UNEX missions are designed for rapid turnaround with fixed budgets in the $10 million US dollar range. The CHIPS project was selected in 1998. The CHIPS mission has passed the Concept Study and Confirmation Reviews. Many lessons have already been learned from the CHIPS UNEX project. This paper will discuss the early issues surrounding the use of commercial satellite constellations as the bus and the politics of small satellites using foreign launchers. The difficulties of finding a spacecraft in the UNEX price range will be highlighted. The advantages of utilizing Internet technologies from the earliest phases of the project through to communications with the spacecraft on orbit will be discussed. The current state of the program, as of July 2001, will be summarized and the project's plans for the future will be charted.     

SETI in the light of cosmic convergent evolution

Theodosius Dobzhansky, one of the founding fathers of the modern evolutionary synthesis, once famously stated that “nothing makes sense in biology except in the light of evolution”. Here it will be argued that nothing in astrobiology makes sense except in the light of “Cosmic Convergent Evolution” (CCE). This view of life contends that natural selection is a universal force of nature that leads to the emergence of similarly adapted life forms in analogous planetary biospheres. Although SETI historically preceded the rise of astrobiology that we have witnessed in the recent decade, one of its main tenets from the beginning was the convergence of life on a cosmic scale toward intelligent behavior and subsequent communication via technological means. The question of cultural convergence in terms of symbolic exchange, language and scientific capabilities between advanced interstellar civilizations has been the subject of ongoing debate. However, at the core of the search for extraterrestrial intelligence lies in essence a biological problem since even post-biological extraterrestrial intelligences must have had an origin based on self-replicating biopolymers. Thus, SETI assumes a propensity of the Universe towards biogenesis in accordance with CCE, a new evolutionary concept which posits the multiple emergence of life across the Cosmos. Consequently, we have to wonder about the biophilic properties the Universe apparently exhibits, as well as to try to find an encompassing theory that is able to explain this “fine-tuning” in naturalistic terms. The aims of this paper are as follows: 1) to emphasize the importance of convergent evolution in astrobiology and ongoing SETI research; 2) to introduce novel and biology-centered cosmological ideas such as the “Selfish Biocosm Hypothesis” and the “Evo Devo Universe” as valuable arguments in theorizing about the origin and nature of extraterrestrial intelligence and 3) to synthesize these findings within an emerging post-biological paradigm on which future SETI efforts may be founded.     

An international relations perspective on the consequences of SETI

Can we envision what the laws of politics and the laws of ethics will be in extraterrestrial civilizations? The laws of physics and chemistry will be the same. Presumably, if there are biospheres in other solar systems, the nature of biology will be the same. Over time evolution may produce the same forms of consciousness and intelligence as we see on earth. However, the political and ethical systems on earth are diverse. Often our images of extraterrestrial civilizations are mere projections of earthly patterns of conflict and cooperation. Perhaps over time the many civilizations and patterns on earth will evolve into one global civilization with harmonious political and ethical norms. These may be the same in universal civilizations if evolution is a cosmic process.     

The temporal aspect of the drake equation and SETI

We critically investigate some evolutionary aspects of the famous Drake equation, which is usually presented as the central guide for research on extraterrestrial intelligence. It is shown that the Drake equation tacitly relies on unverified assumptions on both the physicochemical history of our galaxy and the properties of advanced intelligent communities. In this manner, the conventional approach fails to take into account various evolutionary processes forming prerequisites for quantification of the Drake equation parameters. The importance of recent results of Lineweaver and collaborators on chemical build-up of inhabitable planets for the search for extraterrestrial intelligence is emphasized. Two important evolutionary effects are briefly discussed, and the resolution of the difficulties within the context of the phase-transition astrobiological models is sketched.     

华航大学生学习的现状

大学阶段是学生学习专业知识的开始,是掌握一技之长的重要时期。由于大学生的学习相对独立、内容多、进度快,而且学习与就业息息相关,所以需要学校认真研究大学生的学习,了解大学生学习中存在的问题,给予相应的指导。     

A novel SETI strategy targeting the solar focal regions of the most nearby stars

Many hypotheses have been raised to explain the famous Fermi paradox. One of them is that self-replicating probes could have explored the whole Galaxy, including our Solar System, and that they are still to be detected. In this scenario, it is proposed here that probes from neighboring stellar systems could use the stars they orbit as gravitational lenses to communicate efficiently with each other. Under this hypothesis, a novel SETI approach would be to monitor the solar focal regions of the most nearby stars to search for communication devices. The envisioned devices are probably not detectable by imagery or stellar occultation, but an intensive multi-spectral monitoring campaign could possibly detect some communication leakages. Another and more direct option would be to message the focal regions of nearby stars in an attempt to initiate a reaction.     

NASA的智能协同系统

文章首先概述了智能协同系统在美国航空航天局(NASA)的应用情况,并以NASA普遍使用的两个典型软件工具PMT和NX为例,阐述了智能协同系统的基本功能和技术实现方法,为国内的智能化协同系统软件方面的研究提供参考。     

A SETI metapolicy: New directions towards comprehensive policies concerning the detection of extraterrestrial intelligence

At present we have only one agreed public policy for handling the detection of an extraterrestrial intelligence (ETI), the ‘First SETI Protocol’ of 1989, which guides action in the immediate aftermath of detection, even though SETI (the Search for Extraterrestrial Intelligence) constitutes an active search for such a detection. The purpose of this paper is to set out areas in which policies might fruitfully be developed, including reviewing the rationale and investment in SETI, handling ETI artefacts, and approaches to direct contact. ‘Negative’ possibilities will be examined, for example, whether an ETI artefact or data should be purposefully destroyed.     

A symbiotic approach to SETI observations: use of maps from the Westerbork Synthesis Radio Telescope

High spatial resolution continuum radio maps produced by the Westerbork Synthesis Radio Telescope (WSRT) of The Netherlands at frequencies near the 21 cm HI line have been examined for anomalous sources of emmission coincident with the locations of nearby bright stars. From a total of 542 stellar positions investigated, no candidates for radio stars or ETI signals were discovered to formal limits on the minimum detectable signal ranging from 7.7 x 10(-22) W/m2 to 6.4 x 10(-24) W/m2. This preliminary study has verified that data collected by radio astronomers at large synthesis arrays can profitably be analysed for SETI signals (in a non-interfering manner) provided only that the data are available in the form of a more or less standard two dimensional map format.     

NASA人体研究项目进展分析(上)

人体研究项目是2005年美国航空航天局(NASA)根据美国空间探索新构想而启动的一项研究计划。人体研究项目主要通过国际空间站医学研究、空间辐射、航天员健康对抗措施、探索医学能力、空间人的因素和适居性、行为健康与绩效这六个方面的研究来减少航天员健康和绩效的风险,并以此建立航天员航天飞行健康标准的依据基础。几年来,NASA人体研究项目顺利进行。本文主要分析了近年来人体研究项目的主要进展和主要研究成果。     

NASA人体研究项目进展分析(下)

<正>四、利用非侵入式医学评估系统,不断提高探索任务中的医疗保健能力(ExMC)在月球和火星探索飞行任务中,航天员乘员组不仅需要有维持健康的能力,还需要具备诊断和治疗伤病的能力。探索飞行任务中的医疗保健能力主要是研发飞行任务中的医疗技术、数据处理能力以及不同级别保健的临床措施。医疗技术不仅包括飞行中的诊断和治疗技术,还包括数据系统。     

职业技术学院教职工应付方式的现状调查

了解职业技术学院教职工应付方式现状,采用应付方式问卷(CSQ)对三所职业技术学院的教职工进行调查。结果:职业技术学院教职工使用最多的应付方式是"解决问题";不同性别的教职工在"自责"、"求助"、"幻想"和"合理化"因子上差异有统计学意义(P<0.05);不同工龄的教职工在"解决问题"因子上差异有统计学意义(P<0.05);不同学历的教职工在"合理化"因子上差异有统计学意义(P<0.05);不同职称的教职工在"解决问题"、"求助"、"退避"和"合理化"因子上差异有统计学意义(P<0.05)。结论:应根据职业技术学院教职工应付方式特点进行科学指导。     

Competing for a future in space: NASA and the Department of Defense

Although the 1958 Space Act stressed the civilian nature of the US space programme, the military space budget has grown to over twice the size of NASA's. Military influence on US space policy has grown accordingly. NASA has failed in articulating a sense of direction and purpose for the civilian space programme justifying sustained and adequate support. What matters most for a reinvigorated NASA is the level of commitment the nation is prepared to make, and in today's political climate greater spending on a civilian space programme would be unpopular. The USA looks likely to continue to fall behind in the international competition for space leadership.     

Polarization Studies of Contribution of Aerosol Scattering to the Glow of Twilight Sky

The paper is devoted to studies and a quantitative estimation of the influence of scattering of direct solar radiation by particles of tropospheric aerosols in the period of light twilight, close to sunrise and sunset. Polarization measurements of the twilight sky in two broad spectral bands lying near the standard bands V and R form the basis of these studies. The measurements were carried out in 2002 and 2003 at the Southern Laboratory (Crimea) of the Sternberg Astronomical Institute. The twilight period during which the single aerosol scattering becomes significant is isolated. The character of its influence on the intensity and polarization of the twilight sky is demonstrated. A method is suggested to evaluate polarization of the single aerosol scattering and its contribution to the general brightness of the twilight sky background. The method is based on differential characteristics of the background near the zenith and on their correlations with each other.