Results of the VEGA 1 balloon nephelometer experiment

Backscatter nephelometer measurements obtained during the VEGA 1 balloon flight are reported. During periods of minor convective activity and initial balloon ascent, the data generally agree with those obtained from other Venus mission descent probes. However, during the period of greatest convective activity experienced by the VEGA 1 balloon, the signals were about a factor of two greater than any previously obtained. Although the clouds appear to be unbroken, deviations in the behavior of the detailed backscatter signals with time from those of the ambient pressure or temperature signals, especially during periods of minor convective activity, indicate much small-scale variability in cloud structure.     

变革企业生产方式搞好国营大中型企业

本文从我们课题研究中阐明的企业生产方式的概念出发,从一个新的角度思考搞好国营大中型企业问题。本文认为社会主义企业生产方式内在矛盾的分析应是探讨当前国营大中型企业活力不强、效益不高的重要途径,所以搞好大中型企业的最终出路在于变革企业生产方式,当务之急则是转换企业经营机制。     

Opportunities from space

This article reports on two of the main sessions at the “Space: Technology and Opportunity” conference, Geneva, May 1985, organized by Online Conferences Ltd, Pinner Green House, Ash Hill Drive, Pinner, Middlesex HA5 2AE, UK, from whom the proceedings are available.     

Studies of radio frequency interference at Parkes Observatory

During 16 weeks of continuous SETI observing at the Parkes Observatory in New South Wales, Australia, a set of time-averaged data with 643 Hz resolution were recorded and returned to the SETI Institute for post-processing. These data are the 14 second (10 frame) average powers in each of 15,552 “subband” channels covering 10 MHz of the spectrum in both right and left circular polarizations that were used by the signal detection hardware to baseline and threshold the 1 Hz high resolution SETI spectra. The observations covered frequencies from 1.2 to 3 GHz, tracking 209 stellar targets across the sky. The data at each frequency were averaged over all directions and then interrogated to attempt to determine the prevalence of radio frequency interference (RFI). Estimates were made for the probability of encountering RFI at a particular frequency. Particular attention has been paid to those portions of the spectrum that are allocated as primary use status, or footnote protection for radioastronomy. This sixteen-week snapshot of the RFI situation at Parkes is by now out of date. Unfortunately, a year later, the situation has undoubtedly worsened.     

大学生马克思主义信仰教育:问题与对策

本文在调查研究的基础上对大学生的马克思主义信仰状况进行了分析,找出了理性信仰感性化、信仰分布多元化、入党动机功利化、理论教育不得力等问题.问题的原因有理论教育队伍的素质与教育目标的要求不相适应,教育的方式方法与目标要求不相适应,应试教育的弊端、就业的压力与迷茫、多元信息的吸引与诱惑,马克思主义在大学生信仰中的地位悄然变化等.相应的思路与对策有切实加强师资队伍建设,切实把信仰教育纳入社会系统工程,切实加强党风廉政建设、消除腐败现象对信仰教育的负面影响,切实提高大学生信仰选择能力.     

大学生马克思主义信仰教育：问题与对策

本文在调查研究的基础上对大学生的马克思主义信仰状况进行了分析，找出了理性信仰感性化、信仰分布多元化、入党动机功利化、理论教育不得力等问题。问题的原因有理论教育队伍的素质与教育目标的要求不相适应，教育的方式方法与目标要求不相适应，应试教育的弊端、就业的压力与迷茫、多元信息的吸引与诱惑，马克思主义在大学生信仰中的地位悄然变化等。相应的思路与对策有切实加强师资队伍建设，切实把信仰教育纳入社会系统工程，切实加强党风廉政建设、消除腐败现象对信仰教育的负面影响，切实提高大学生信仰选择能力。     

Estimates of convective heat fluxes and gravity wave amplitudes in the Venus middle cloud layer from VEGA balloon measurements

Atmospheric temperatures and vertical velocities obtained from the VEGA balloon measurements indicate that the dynamical heat flux is upward and has an amplitude that ranges from 0 to 360 W m⁻² in the middle cloud region. The static stability is positive and ranges from 0 to 2.0 K km⁻¹. Time series analysis of these results indicates that convection is the principal mechanism for generating the large vertical motions. Gravity waves were also detected at these levels and account for about 15% of the covariance between temperature and vertical velocity.     

The Progress of the Taiwan Oscillation Network Project

We describe the present status of the project of the Taiwan Oscillation Network (TON) and discuss a scientific result using the TON data. The TON is a ground-based network to measure solar intensity oscillations for the study of the solar interior. Four telescopes have been installed in appropriate longitudes around the world. The TON telescopes take K-line full-disk solar images of diameter 1000 pixels at a rate of one image per minute. The data has been collected since October of 1993. The TON high-spatial-resolution data are specially suitable for the study of local properties of the Sun. In 1997 we developed a new method, acoustic imaging, to construct the acoustic signals inside the Sun with the acoustic signals measured at the solar surface. From the constructed signals, we can form intensity map and phase-shift map of an active region at various depths. The direct link between these maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximation. This technique of acoustic imaging has been used to image the far-side of the Sun that could provides information on space weather prediction. The TON Team includes: Antonio Jimenez (Instituto Astrofisica de Canarias, Spain); Guoxiang Ai and Honqi Zhang (Huairou Solar Observing Station, P.R.C.); Philip Goode and William Marquette (Big Bear Solar Observatory, U.S.A.); Shuhrat Ehgamberdiev and Oleg Ladenkov (Ulugh Beg Astronomical Institute, Uzbekistan) This revised version was published online in August 2006 with corrections to the Cover Date.     

经营目标与产权结构

本文从产业组织理论出发,以企业产权结构的变革为前提,阐述和讨论了H—型、U—型和M—型股份制企业经营目标和行为目标的变异。