Rotation measure variations for 20 millisecond pulsars     

W. M. Yan  R. N. Manchester  G. Hobbs  W. van Straten  J. E. Reynolds  N. Wang  M. Bailes  N. D. R. Bhat  S. Burke-Spolaor  D. J. Champion  A. Chaudhary  W. A. Coles  A. W. Hotan  J. Khoo  S. Oslowski  J. M. Sarkissian  D. R. B. Yardley 《Astrophysics and Space Science》2011,335(2):485-498

We report on variations in the mean position angle of the 20 millisecond pulsars being observed as part of the Parkes Pulsar Timing Array (PPTA) project. It is found that the observed variations are dominated by changes in the Faraday rotation occurring in the Earth??s ionosphere. Two ionospheric models are used to correct for the ionospheric contribution and it is found that one based on the International Reference Ionosphere gave the best results. Little or no significant long-term variation in interstellar RM was found with limits typically about 0.1 rad?m^?2?yr^?1 in absolute value. In a few cases, apparently significant RM variations over timescales of a few 100 days or more were seen. These are unlikely to be due to localised magnetised regions crossing the line of sight since the implied magnetic fields are too high. Most probably they are statistical fluctuations due to random spatial and temporal variations in the interstellar electron density and magnetic field along the line of sight.  相似文献   

A stochastic ground motion model with separable temporal and spectral nonstationarities     

Sanaz Rezaeian  Armen Der Kiureghian 《地震工程与结构动力学》2008,37(13):1565-1584

A fully nonstationary stochastic model for strong earthquake ground motion is developed. The model employs filtering of a discretized white‐noise process. Nonstationarity is achieved by modulating the intensity and varying the filter properties in time. The formulation has the important advantage of separating the temporal and spectral nonstationary characteristics of the process, thereby allowing flexibility and ease in modeling and parameter estimation. The model is fitted to target ground motions by matching a set of statistical characteristics, including the mean‐square intensity, the cumulative mean number of zero‐level up‐crossings and a measure of the bandwidth, all expressed as functions of time. Post‐processing by a second filter assures zero residual velocity and displacement, and improves the match to response spectral ordinates for long periods. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

Solar Image Restoration By Use Of Multi-frame Blind De-convolution With Multiple Objects And Phase Diversity     

Michiel Van Noort  Luc Rouppe Van Der Voort  Mats G. Löfdahl 《Solar physics》2005,228(1-2):191-215

An extension of Joint Phase Diverse Speckle image restoration is presented. Multiple realizations of multiple objects having known wavefront relations with each other can now be restored jointly. As the alignment of the imaging setup does not change, near-perfect alignment can be achieved between different objects, thus greatly reducing false signals in the determination of derived quantities, such as magnetograms, Dopplergrams, etc. The method was implemented in C++ as an image restoration server, to which worker clients can connect and disconnect randomly, so that a large number of CPUs can be used to speed up the restorations. We present a number of examples of applications of the restoration method to observations obtained with the Swedish 1-m Solar Telescope on La Palma.  相似文献   

Frequency dependence of Q in the mantle underlying the shield areas of Eurasia, Part II: analyses of long period data     

Alison C. Lees  Zoltan A. Der  Vernon F. Cormier  Margaret E. Marshall  James A. Burnetti 《Geophysical Journal International》1986,87(3):1085-1101

  相似文献   

BiSON performance     

William J. Chaplin  Yvonne Elsworh  Rachel Howe  George R. Isaak  Clive P. McLeod  Brek A. Miller  H. B. Van Der Raay  Sarah J. Wheeler  Roger New 《Solar physics》1996,168(1):1-18

Since 1981 we have been operating the Birmingham Solar-Oscillations Network (BiSON), a global network of resonant-scattering spectrometers, observing the low-l solar p modes. Here we discuss historical developments, culminating in the establishment of a 6-station network in 1992 September, and the subsequent performance of that network. The data record of each station from 1992 to 1994 has been analysed in terms of weather and equipment breakdowns. Our early experience suggests that the best long-term coverage possible with a 6-station network is limited in practice to about 80%, which falls short of previous predictions.  相似文献   

Einladung zur Hauptversammlung am Samstag,den 4. Januar 1913, nachmittags 3 Uhr     

Der Vorstand 《International Journal of Earth Sciences》1912,3(7):519-520

Ohne ZusammenfassungAnmeldungen zu weiteren Vorträgen bittet man an Herrn Dr.Drevermann, Frankfurt a. M., Victoriaallee 7, zu richten.  相似文献   

Bücher- und Zeitschriftenschau     

Hummel  St  Rüger  Wcks  Der 《International Journal of Earth Sciences》1924,15(2):175-187

Ohne Zusammenfassung  相似文献   

o,p′-DDT induction of vitellogenesis and its inhibition by tamoxifen in Nile tilapia (Oreochromis niloticus)     

Olga Leaos-Castaeda  Glen Van Der Kraak  Andrea Lister  Raúl Sim-Alvarez  Gerardo Gold-Bouchot 《Marine environmental research》2002,54(3-5)

In order to investigate the mechanism by which o,p′-DDT disrupts endocrine functioning of Nile tilapia in vivo, the estrogenicity of o,p′-DDT was investigated in conjunction with 17β-estradiol (E₂) and tamoxifen. Mature, male tilapia were treated intraperitoneally with o,p′-DDT (60 mg/kg, one dose) or E₂ (5 mg/kg, four doses) in the presence or absence of tamoxifen (5 mg/kg, six doses) for 12 days and then plasma vitellogenin (Vtg) (measured as alkaline-labile phosphorous), E₂, and testosterone (T) were measured. Vtg levels were increased dramatically by E₂ (1744±171 μg/ml) and moderately by o,p′-DDT (82±15 μg/ml) compared with controls (23±3.5 μg/ml). Tamoxifen alone had no effect on Vtg production, but inhibited both E₂ and o,p′-DDT stimulated vitellogenesis. T levels were reduced with E₂ administration (1688±383 pg/ml) and declined further with the combined treatment of E₂ and tamoxifen (281±70 pg/ml), compared with controls (6558±1438 pg/ml). Tamoxifen or o,p′-DDT alone did not affect T levels, but their combined treatment did (2069±647 pg/ml). The results of this study suggest that o,p′-DDT is weakly estrogenic in male tilapia, and that this activity may be mediated through the estrogen receptor.  相似文献   

Multifrequency study of the nuclei of Sbc galaxies     

M. B. Vila  R. D. Davies  A. Pedlar  D. J. Axon  E. Hummel  J. M. Van Der Hulst 《Astrophysics and Space Science》1989,157(1-2):277-286

A sample of 100 Sbc galaxies has been observed at different wavelengths and resolutions. The ultimate aim of the project is to probe the origin of their nuclear activity, e.g., blackhole, starbust, etc.The results from radio observations with the VLA (New Mexico) at 20 and 6 cm, with a resolution of 1–2 arc sec, for the inner kpc of nineteen sources are presented. Six of the galaxies show extended emission consistent with starburst activity. The remaining thirteen are unresolved or marginally resolved compact sources. Their steep spectra indicate synchrotron emission. They show total nuclear energies similar to those found for a sample of Seyfert galaxies.Optical spectroscopic observations with a similar resolution to the radio data have been made for approximately 90 galaxies. A sample of the derived rotation curves is included.  相似文献   

塔里木盆地中南部麻扎塔格逆冲—褶皱带变形特征及其意义   总被引：1，自引：0，他引：1       下载免费PDF全文

潘家伟  李海兵  孙知明  裴军令  司家亮  Laurie Barrier  邱祝礼  吴富峣  张丽军 《地质科学》2010,45(4):1038-1056

麻扎塔格地区地层、地貌及构造变形特征的研究,对于认识塔里木盆地新生代构造演化过程、塔里木—西昆仑的盆山耦合关系、新构造运动对塔里木油气资源分布的影响以及塔克拉玛干沙漠的气候、环境变化都具有重要意义。本文通过卫星照片解译、野外变形观察、剖面实测、地球物理资料解释等手段,对该地区晚新生代的构造特征进行了研究,确定了麻扎塔格构造带为典型的逆冲—褶皱带,并探讨了麻扎塔格逆冲—褶皱带的构造指向、活动时限、隆升速率及缩短速率、东西方向的延伸等问题,取得如下认识:1)麻扎塔格逆冲—褶皱带为西昆仑山前陆褶皱冲断带的前缘部位,和田河气田就是处在逆冲前锋背斜顶部,晚新生代变形作用已明显地改造了塔里木盆地南部及中部的古生代和中生代构造,并促成了和田河气田的形成;2)麻扎塔格山在中新世末(约7 Ma)和中更新世(约780 ka B.P.)经历了两次构造隆升,后一次形成了麻扎塔格逆冲—褶皱带和麻扎塔格山现今的地貌特征;3)估算出麻扎塔格逆冲—褶皱带中更新世以来的隆升速率约为0.26～0.4 mm/a,缩短速率约为0.9 mm/a;4)认为麻扎塔格逆冲—褶皱带向西应与同属西昆仑山前褶皱—冲断带前缘的喀什背斜相连,东端的突然消失可能是由于东段和田河附近存在北东—南西向的走滑断层造成。  相似文献