昆明1943年5级地震的发震地段考证

结合资料记载与调查,认为该地震发生在昆明市区西南边缘的西山断裂地段。     

印尼8.7级巨震后云南地震活动的频度变化

0引言 2004年12月26日在印尼苏门答腊西北近海发生了8．7级巨震，3月29日在距8．7级地震破裂区东南160km又发生了一次8．5级地震。8．7级地震发生后，余震向震中以北扩展达千米以上。如此剧烈的能量释放，对我国的地震活动有何影响是令人关注的，但清晰解答这个问题并非易事，主要原因是，一个地区的大地震发生后如何影响另一个地区地震活动的机制目前我们并不清楚。这个机制可能很复杂，涉及到应力在地壳和地幔内的传播、积累，以及与地质构造等的关系。因此，仅从时间尺度上判定一个地区的大地震对另一个地区地震活动是否有影响在认识上就存在分歧。例如，是一个地区的大地震发生后的波动在传播到另一个地区时直接触发的地震活动才被看作是影响？还是由于一个地区的大地震发生后的应力释放和调整影响到另一个地区的地震活动才被看作是影响？显然，这两方面的影响在时间尺度上存在差异。8．7级地震发生后不到20分钟，在我国云南的宾川发生了4．6级地震，其发震时间也是8．7级地震的面波到达该地区的时间（李刚等，2005）；     

TRIFFID Photometry of Globular Cluster Cores — I. Photometric Techniques and Variable Stars in M15

The Galway/DIAS Image Sharpening Camera, TRIFFID, has been used to make observations in two colours of the centre of the post-core-collapse globular cluster M15. We present here our analysis of the photometry in B over two seasons. We have combined the complementary qualities of the HST 's high astrometric precision and TRIFFID's extended coverage and photometric precision, to perform crowded-field photometry in the innermost region of M15. Our technique virtually eliminates the problem of extreme crowding which has hitherto hampered studies of the variable star populations in globular cluster cores, and thereby provides an extension of the HST 's capability. Candidate variables detected with the HST have been confirmed and monitored over longer periods. We show that most of these are RR Lyrae stars, and that one is a short-period Type II Cepheid (the third to be discovered in M15). Our photometric study also produced evidence of a similar number of new variables. These also appear to be RR Lyrae stars, except for a possible eclipsing system. Further data from an upgraded version of TRIFFID have recently been obtained to help to refine the light curves of all these objects.     

Statistical properties of H II regions in the disc of M100

From a new mosaic image in the Hα line of the complete disc of the spiral galaxy M100, a catalogue is composed listing 1948 individual H II regions. I give details of the data collection and reduction procedure, and of the production of the H II region catalogue. For each H II region, the catalogue gives its position relative to the centre of the galaxy, its deprojected distance to the centre, its radius and its calibrated luminosity. An indication is included as to whether the H II region is located in the arms, between them, or in the circumnuclear star-forming region. I present the results of a statistical study of properties of the H II regions. The luminosity function of the complete ensemble of H II regions shows a characteristic shape well fitted by a power-law slope in the higher luminosity range, and complying with literature values for galaxies like M100. Luminosity function slopes for arm and interarm H II region populations separately are found to be equal within the errors of the fits, indicating that whereas the density wave accumulates material into the arm regions, and may trigger star formation there, it does not in fact change the mass distribution of the star-forming clouds, nor the statistical properties of the H II region population. Diameter distributions and the radial number density distribution are discussed. The latter indicates those areas where most star formation occurs: the circumnuclear region and the spiral arms. The huge number of H II regions allowed the construction of a number of independent luminosity functions at different distances to the nucleus. The slope of the luminosity function shows a marginal decrease with increasing distance from the centre, which could indicate a gradual change towards shallower IMF slopes with increasing galactocentric distance, or an evolutionary effect.     

Chlorinated hydrocarbons in gulls from the Baltic south coast

Polychlorinated terphenyls among organochlorine pesticides and polychlorinated biphenyls were detected in some gulls from the Gdańsk Bay, Baltic Sea.     

Recent discoveries of supersoft X‐ray sources in M 31

Classical novae (CNe) have recently been reported to represent the major class of supersoft X‐ray sources (SSSs) in the central area of our neighbouring galaxy M 31. This paper presents a review of results from recent X‐ray observations of M 31 with XMM‐Newton and Chandra. We carried out a dedicated optical and X‐ray monitoring program of CNe and SSSs in the central area ofM 31. We discovered the first SSSs in M 31 globular clusters (GCs) and their connection to the very first discovered CN in a M 31 GC. This result may have an impact on the CN rate in GCs. Furthermore, in our optical and X‐ray monitoring data we discovered the CN M3 1N 2007‐11a, which shows a very short SSS phase of 29–52 days. Short SSS states (durations ≤ 100 days) of CNe indicate massive white dwarfs (WDs) that are candidate progenitors of supernovae type Ia. In the case of M31N 2007‐11a, the optical and X‐ray light curves suggest a binary containing a WD with M_WD > 1.0 M_⊙. Finally, we present the discovery of the SSS counterpart of the CN M31N 2006‐04a. The X‐ray light curve of M31N 2006‐04a shows short‐time variability, which might indicate an orbital period of about 2 hours (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

汶川8.0级大地震震源机制与构造运动特征

根据地震震源机制、断层参数结果,结合GPS测定的同震位移场与构造研究的最新结果,综合分析研究了2008年汶川8级大地震汶川地震发生的地震活动背景、震源应力场、断层构造运动特征及其动力学机制。地震活动性分析研究结果表明,2008年汶川8级大地震是在青藏高原与其周边地域构造运动剧烈,2001年起始的地震活动高潮期的背景下发生的。其长达300km的地震震源断层填补了青藏高原东缘1900年以来存在的8级地震活动的空区。震源机制与区域应力场特征及其动力学机制研究表明,汶川8级地震震源处于南北地震带中南段东部,青藏高原东向扩张与四川盆地的抵抗是该区构造运动的主要特征。汶川地震及其强余震是在一个稳定的、主压应力P轴以北西西-东南东方向为主的震源应力场控制下发生的。说明汶川地震震源区域主要受到四川盆地、华南块体区域应力场的控制并发震的。龙门山断裂带西侧的青藏高原相对于四川盆地发生的东向上升;而东侧的四川盆地相对于青藏高原发生的西向下降构造运动是2008年汶川8级地震发生的主要地震成因即地震发生机制。