Buildings Damages after Elazığ, Turkey Earthquake on January 24, 2020     

Dogan  Gamze  Ecemis  Ali Serdar  Korkmaz  Serra Zerrin  Arslan  Musa Hakan  Korkmaz  Hasan Husnu 《Natural Hazards》2021,109(1):161-200

A 6.8-magnitude earthquake that occurred on January 24, 2020, has been effective in Turkey’s eastern regions. The earthquake, with recorded peak ground acceleration (PGA) value of 0.292 g, caused the destruction or heavy damage of buildings, especially in the city center of Elaz?? province. The purpose of this paper was to share the results of detailed investigation in the earthquake-stricken area. Additionally, the causes of damages and failures observed in the buildings were compared to those that had occurred in previous earthquakes in Turkey. In this study, the damages observed in especially RC buildings as well as in masonry and rural buildings were summarized, the lessons learned were evaluated, and the results were interpreted with reference to Turkish earthquake codes. In the study, it was particularly emphasized why the building stock underwent such damage even though the buildings were exposed to earthquake acceleration well below the design acceleration values.

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Effects of Slaking fluid pH on the Index Properties of Carbonate Rocks     

Arman  Hasan 《Geotechnical and Geological Engineering》2021,39(8):5843-5855

Geotechnical and Geological Engineering - The physical and chemical characteristics of water critically influence the mechanical and chemical breakdown of rocks. The physical properties of rocks,...  相似文献   

Annual production and productivity of the macrophytes of river Champanala,a side spill channel of the Ganges at Bhagalpur     

R. Hasan 《洁净——土壤、空气、水》1988,16(6):573-578

The present investigation gives the turnover value and productivity of macrophytes like Eichhornia crassipes, Hydrilla verticillata, Ceratophyllum demersum, Potamogeton crispus and Azolla pinnata for the year 1978 at Koylaghat site of the Champanala channel, a southern side spill channel of the river Ganges. The average annual production of all the macrophytes comes to 3.925 g/m² · d, which is better than the world average of rice cultivated fields. All the important macrophytes in the present investigation are replaced annually. In contrast to pond and reservoir ecosystems, where the productivity of macrophytes is highest in the rainy season, in the Champanala channel the most of the macrophytes are absent from July to December and maximal productivity was about 4 g/m² · d from February to April. The difference in the development of macrophytes in standing and flowing waters results from the fact that in the rainy season increasing flow velocity, sudden fluctuations in water column depth and other destabilising factors produce unfavourable conditions for macrophytes in flowing waters.  相似文献   

Lessons learnt from checking the quality of openly accessible river flow data worldwide     

L. Crochemore  K. Isberg  R. Pimentel  L. Pineda  A. Hasan  B. Arheimer 《水文科学杂志》2020,65(5):699-711

ABSTRACT

Advances in open data science serve large-scale model developments and, subsequently, hydroclimate services. Local river flow observations are key in hydrology but data sharing remains limited due to unclear quality, or to political, economic or infrastructure reasons. This paper provides methods for quality checking openly accessible river-flow time series. Availability, outliers, homogeneity and trends were assessed in 21 586 time series from 13 data providers worldwide. We found a decrease in data availability since the 1980s, scarce open information in southern Asia, the Middle East and North and Central Africa, and significant river-flow trends in Africa, Australia, southwest Europe and Southeast Asia. We distinguish numerical outliers from high-flow peaks, and integrate all investigated quality characteristics in a composite indicator. We stress the need to maintain existing gauging networks, and highlight opportunities in extending existing global databases, understanding drivers for trends and inhomogeneity, and in innovative acquisition methods in data-scarce regions.  相似文献   

NASA's Astrophysics Data Archives     

H. Hasan  R. Hanisch  J. Bredekamp 《Astrophysics and Space Science》2000,273(1-4):131-139

The NASA Office of Space Science has established a series of archivalcenters where science data acquired through its space science missionsis deposited. The availability of high quality data to the generalpublic through these open archives enables the maximization of sciencereturn of the flight missions. The Astrophysics Data Centers CoordinatingCouncil, an informal collaboration of archival centers, coordinates datafrom five archival centers distiguished primarily by the wavelength rangeof the data deposited there. Data are available in FITS format. Anoverview of NASA's data centers and services is presented in this paper.A standard front-end modifyer called Astrowbrowse is described. Othercatalog browsers and tools include WISARD and AMASE supported by theNational Space Scince Data Center, as well as ISAIA, a follow on toAstrobrowse.  相似文献   

近14 a也门降水异常的气候特征   总被引：2，自引：0，他引：2  

加买尔  龚  陆维松 《南京气象学院学报》2006,29(6):847-849

利用1990-2003年也门7个测站降水资料，在分析近148也门降水季节变化特征的基础上，着重分析了也门夏季降水的年际变化特征。结果表明，也门降水异常的季节变化明显，异常在4-9月最大，尤其是7-9月，异常峰值所在月呈现出较明显的提早趋势；近148也门夏季降水呈现出增加的趋势，90年代末该趋势加大；近148也门夏季降水存在38和78左右的显著振荡周期。  相似文献   

近14a也门降水异常的气候特征          下载免费PDF全文

加买尔  龚  陆维松 《大气科学学报》2006,29(6):847-849

利用1990-2003年也门7个测站降水资料,在分析近14 a也门降水季节变化特征的基础上,着重分析了也门夏季降水的年际变化特征。结果表明,也门降水异常的季节变化明显,异常在4-9月最大,尤其是7-9月,异常峰值所在月呈现出较明显的提早趋势;近14 a也门夏季降水呈现出增加的趋势,90年代末该趋势加大;近14 a也门夏季降水存在3 a和7 a左右的显著振荡周期。  相似文献   

Morphologies of AGN host galaxies using HST/ACS in the CDFS-GOODS field     

Priya Hasan 《Astrophysics and Space Science》2007,312(1-2):63-77

Using HST/ACS images in four bands F435W, F606W, F775W and F850LP, we identify optical counterparts to the X-ray sources in the Chandra Deep Field South in the GOODS South field. A detailed study has been made of these sources to study their morphological types. We use methods like decomposition of galaxy luminosity profiles, color maps and visual inspection of 192 galaxies which are identified as possible optical counterparts of Chandra X-ray sources in the CDFS-GOODS field. We find that most moderate luminosity AGN hosts are bulge dominated in the redshift range (z≈0.4–1.3), but not merging/interacting galaxies. This implies probable fueling of the moderate luminosity AGN by mechanisms other than those merger driven.  相似文献   

RAGLAND,AN LL3.4 CHONDRITE FIND FROM NEW MEXICO     

S.I. Recca  E.R.D. Scott  K. Keil  R.N. Clayton  T.K. Mayeda  G.I Huss  E. Jarosewich  K.S. Weeks  F.A. Hasan  D.W.G. Sears  R. Wieler  P. Signer 《Meteoritics & planetary science》1986,21(2):217-229

The Ragland, New Mexico chondrite was found in 1978, and consists of a single stone of 12.16 kg that broke into three pieces. The stone is moderately weathered and has a pronounced chondritic texture. Bulk composition favors an LL classification, and modal analysis and oxygen isotopic composition are consistent with this. The thermoluminescence sensitivity of 0.056 ± 0.020 normalized to Dhajala, compositional variability of olivine (mean Fa 18.3, σ = 10.1) and low-Ca pyroxene (mean Fs 14.6, σ = 6.7), and Ca concentrations in olivine indicate metamorphic subtype 3.4 ± 0.1. The isotopically heavy oxygen composition, which is characteristic of subtypes 3.0–3.1, may be a primary characteristic and not a result of weathering. Low concentrations of radiogenic ⁴⁰Ar and planetary ³⁶Ar suggest noble gas loss.  相似文献   

Stokes Diagnostics of Magneto-Acoustic Wave Propagation in the Magnetic Network on the Sun     

G. Vigeesh  O. Steiner  S. S. Hasan 《Solar physics》2011,273(1):15-38

The solar atmosphere is magnetically structured and highly dynamic. Owing to the dynamic nature of the regions in which the magnetic structures exist, waves can be excited in them. Numerical investigations of wave propagation in small-scale magnetic flux concentrations in the magnetic network on the Sun have shown that the nature of the excited modes depends on the value of plasma β (the ratio of gas to magnetic pressure) where the driving motion occurs. Considering that these waves should give rise to observable characteristic signatures, we have attempted a study of synthesised emergent spectra from numerical simulations of magneto-acoustic wave propagation. We find that the signatures of wave propagation in a magnetic element can be detected when the spatial resolution is sufficiently high to clearly resolve it, enabling observations in different regions within the flux concentration. The possibility to probe various lines of sight around the flux concentration bears the potential to reveal different modes of the magnetohydrodynamic waves and mode conversion. We highlight the feasibility of using the Stokes-V asymmetries as a diagnostic tool to study the wave propagation within magnetic flux concentrations. These quantities can possibly be compared with existing and new observations in order to place constraints on different wave excitation mechanisms.  相似文献