用瑞雷和乐夫面波羣速度确定我国地壳厚度

一、方法及所用資料本文根据三十九个地震,利用基型面波羣速度的方法,确定了我国东半部、浅海区及西藏高原东部的地壳厚度。所用資料包括我国十个基本地震台上基式地震仪的記录,选用地震的震級均为5級以上,除个別地震外均为浅源地震。     

保角映射在換算重磁观测資料中的某些应用

本文利用保角映射方法对两种二维地形作了推导:一种是半圆弧形的边界,另一种是拋物线形的边界。并作了一些数值计算。     

Zur Revision der GattungGloeocapsa Kützing (Cyanophyta)

Ohne Zusammenfassung Die vorliegende Arbeit entstand dank der Unterstützung der Alexander-von-Humboldt-Stiftung, Bad Godesberg.     

金属矿床直流电法勘探的几个问题

本文討論了几种干扰因素（包括地形、地表和地下的局部不均勻以及围岩的非各向同性等）对地下直流电場的影响規律及如何避免这种影响的問題。根据作者初步研究的結果,对克服干扰影响和确定矿体产状要素等提出了某些方法及其理論依据。     

水平旋转椭球体的自然电场及其解释

引言在前一篇文章中,我們討論了繞垂直軸旋轉橢球體的自然電場和解釋。本文將討論水平旋轉橢球體的自然電場和其解釋方法。水平旋轉橢球體的自然電场 設垂直極化的水平旋轉橢球體位在一均匀各向同性無限大的介質里,其電阻率為     

Some foundation stability problems of the railway bridge over the Mala Rijeka

SummarySome Foundation Stability Problems of the Railway Bridge over the Mala Rijeka The authors presented an outlay of problems occurring in estimating the stability of rocky slopes loaded by large vertical forces. General attitudes, kept by the authors during the stability analysis for an actual case — foundation of piers No. 3 and 4 of the railway bridge across the Mala Rijeka, are also presented. The results of calculation as well as the advantages of the approach applied are outlined in the paper. Finally, general conclusions are drawn regarding the method to be kept in solving the stability of slopes loaded by large artificial loading.With 7 Figures     

New Definition of Discovery for Solar System Objects

We propose a new formal definition of discovery for a Solar System object. It is based on an objective and mathematically rigorous algorithm to assess when a set of observations is enough to constitute a discovery. When this definition is satisfied, in almost all cases the orbit is defined well enough to establish the nature of the object discovered (Main Belt vs. Near Earth Asteroid, Trans-Neptunian vs. long period comet). The frequency of occurrence of exceptions is estimated by a set of numerical experiments. The availability of a non-subjective definition of discovery allows some rules to be adopted for the assignment of discovery credit with a minimum risk of dispute. Such rules should be fair, encourage good practice by the observers and acknowledge the contribution of the orbit computers providing the identifications and the orbits, as well as the one of all the contributing observers.     

Dynamical portrait of the Lixiaohua asteroid family

In this paper we present a comprehensive analysis of the dynamics in the region of the (3556) Lixiaohua asteroid family. The family lies in a particularly interesting region of the phase space, crossed by several two-body and three-body mean motion resonances. Also, members of this family can have close encounters with large asteroids, such as Ceres. We have identified the mean motion resonances which contribute to the long-term dynamical evolution of the family and our results confirm that the members of this family can be classified into a number of groups, exhibiting different dynamical behavior. We show for the first time that in the Lixiaohua region, apart from the chaotic diffusion in proper eccentricity and inclination (e _p and I _p ), there is at least one extended chaotic zone where several resonances overlap, thus giving rise to chaotic diffusion in proper semi-major axis (a _p ) as well. Using a code of Monte Carlo type, we simulate the evolution of the family, according to the model which combines the chaotic diffusion (in a _p , e _p and I _p ), Yarkovsky/YORP thermal effect and random walk in a _p due to the close encounters with massive asteroids. These simulations show that all these effects should be taken into account in order to accurately explain the observed distribution of family members in the space of proper elements, although a “minimal” model that accounts for chaotic diffusion in (e _p , I _p ), Yarkovsky-induced drift in a _p and random walk in a _p due to the close encounters with the most massive asteroids is enough to grossly characterize the shape of the family.