地外生命搜索和太阳系外的行星的发现

阐述地外生命搜索的意义，手段和现状，地外生命搜索的SETI计划及其发展，并着重介绍太阳系外的行星系统的发现，它的目的，成果以及未来。太阳系外的行星系统的发展是当代天文学最时髦的，也将是未来21世纪成果最丰富的研究领域之一，从1992年第一个确认了脉冲星PSR 1257＋12的行星系统以来，1995年确认主序星51Peg有一颗行星，至2001年5月，已经发现了60个太阳系外的行星系统，太阳系外的行星系统的发现与地外生命搜索研究是密不可分的，新的发现也提出了很多新的谜，这项研究近10年来发展很快，它的研究也促进了航天学，宇宙化学，天文生物学乃至哲学等其他学科的发展。     

Implications of mean field accretion disc theory for vorticity and magnetic field growth

In addition to the scalar Shakura–Sunyaev α _ss turbulent viscosity transport term used in simple analytic accretion disc modelling, a pseudo-scalar transport term also arises. The essence of this term can be captured even in simple models for which vertical averaging is interpreted as integration over a half-thickness and each hemisphere is separately studied. The additional term highlights a complementarity between mean field magnetic dynamo theory and accretion disc theory treated as a mean field theory. Such pseudo-scalar terms have been studied, and can lead to large-scale magnetic field and vorticity growth. Here it is shown that vorticity can grow even in the simplest azimuthal and half-height integrated disc model, for which mean quantities depend only on radius. The simplest vorticity growth solutions seem to have scales and vortex survival times consistent with those required for facilitating planet formation. In addition, it is shown that, when the magnetic back-reaction is included to lowest order, the pseudo-scalar driving the magnetic field growth and that driving the vorticity growth will behave differently with respect to shearing and non-shearing flows: the former pseudo‐scalar can more easily reverse sign in the two cases.     

Long-term cyclicity of the Herbig Ae star BF Ori: Giant protocomets and accretion from a protoplanetary disk

Having analyzed the light curve for the Herbig Ae star BF Ori, we justify the hypothesis of a giant protocomet, GPC I BF Ori, with a period of 6.3 years and semimajor axis a = 10 ± 3 AU. Passing through periastron, such a giant protocomet partially breaks up. During each passage through periastron, the protocomet and the fragments that follow it supply dust to circumstellar space for a certain period of time. This hypothesis can account for the entire complex of observable phenomena of cyclic Algol-like activity in Herbig Ae/Be and T Tauri stars. Conditions in a protoplanetary disk after cocoon breakup are discussed. We adduce arguments for the absence of a dust disk and for the weak effect of objects other than comets on cyclic large-scale variability.     

On the internal energy source of the large planets

Based on spacecraft observations of the giant planets we call attention to an apparent regular mass-luminosity relation for the large planets (giant planets plus Earth). It can provide important clues and constraints on the question of their energy source, including various relevant theories and their difficulties. We describe in some detail a new thermonuclear reaction mechanism, valid for plasma fusions at both super—high and low temperatures, and including the original thermonuclear mechanism as a particular case. It can explain not only the internal energy souce of the large planets, but also many anomalous fusion phenomena observed in the laboratory and in astronomical bodies. Although these appear in various guises, their basic principle is the same, that is, they can all be understood in terms of the new mechanism.     

Long term wind erosion on Mars

Wind erosion and deposition are powerful agents of surface change on Mars. Erosion is sensitive to the atmospheric density, so feedback between orbit variations and atmospheric density can enhance the sensitivity of erosion rates to orbital parameters. We use statistics derived from a 1 Gyr integration of the spin axis of Mars, coupled with runs of the NASA Ames 3-D general circulation model (GCM) at a variety of orbital conditions and pressures, to explore this feedback. We find that wind erosion in the GCM is associated with two factors: baroclinic zone winds, and strong cross-equator solstice flows. Both of these factors are influenced by topography, producing an asymmetry in the erosion pattern between the north and the south. The erosion model, averaged over 1 Gyr, produces potential erosion rates of in the north and in the south, which increase by an order of magnitude in an early 28 mbar atmosphere. The stability of these potential erosion patterns over geological time indicates that the lowland regions of Mars are continuously eroded, and that wind is capable of revealing ancient sedimentary deposits, or eroding substantial deposits that may have otherwise been preserved.     

A Cosmological Explanation to the Pioneer Anomaly

An earlier paper introduced a new cosmological theory based on the proposition that all four metrical coefficients of space and time change with the cosmological expansion. Such a universal scale expansion would preserve the four-dimensional spacetime geometry and therefore by general relativity most physical relationships. In addition, if the scale expansion were exponential with time, all epochs would be equivalent. The theory resolves several outstanding problems with the standard model based on the Big Bang concept and better agrees with observations. Four independent observational programs support the SEC theory, which also provides an explanation to the Pioneer anomaly. A possible resolution to the recently discovered discrepancies between optical observations of the planets and their ephemerides is proposed.     

The Eddington Mission

The Eddington mission was given full approval by the European Space Agencyon the 23rd May 2002, as part of the new `Cosmic Vision' Science programme, with launch scheduled for 2007/8. Its twin scienceobjectives are asteroseismology and planet finding.In its current design it consists of 4 × 60 cm folded Schmidt telescopes, eachwith 6° × 6° field of view and its own CCD array camera.The current observing plan is to spend 2 years primarily devoted to asteroseismologywith 1–3 months on different target fields monitoring up to 50,000 stars per field,and 3 years continuously on asingle target field monitoring upwards of 100,000 stars as required for planetsearching. The asteroseismic goal is to be able to detect oscillationsfrequencies with a precision 0.1–0.3 Hz.     

骨巨细胞瘤的影像学诊断

目的：探讨骨巨细胞瘤的影像学表现。资料与方法：对50例各种类型的骨巨细胞瘤的影像学表现进行了分析结果：骨巨细瘤的基本影像表现为：骨端偏心性膨胀骨质破坏,骨皮质薄而完整,骨嵴纤细呈网络状,无骨膜反应,溶骨型者,骨皮质中断,骨嵴减少或消失肿瘤边缘较模糊;恶变者,破坏区的骨干侧出现虫蚀状或筛孔样骨质破坏,有骨膜三角和生长迅速的软组织肿块。结论：骨巨细胞瘤的X线表现具有一定的特征。CT能显示骨巨细胞瘤的内部结构,腰骶部骨巨细胞瘤可显示突向盆腔和腹腔内的软组织块影。     

行星环动力学

行星环动力学的研究对揭示太阳系，星系的形成和演化有重要的意义，旅行者２号的行星际探测，极大地丰富的我们对行星环的认识，给行星环动力学的研究带来了活力，文中综合在行星轴对称势，环自引力势，环粒子磁撞，卫星摄动等因素影响了行星环的研究方法法及研究进展。