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排序方式: 共有257条查询结果,搜索用时 359 毫秒
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Y. Mizumura J. Kushida K. Nishijima G.V. BicknellR.W. Clay P.G. EdwardsS. Gunji S. HaraS. Hayashi S. KabukiF. Kajino A. KawachiT. Kifune R. KiuchiK. Kodani Y. MatsubaraT. Mizukami Y. MizumotoM. Mori H. MuraishiT. Naito M. OhishiV. Stamatescu D.L. SwabyT. Tanimori G. ThorntonF. Tokanai T. ToyamaS. Yanagita T. YoshidaT. Yoshikoshi 《Astroparticle Physics》2012,35(9):563-572
We have searched for very high energy (VHE) gamma rays from four blazars using the CANGAROO-III imaging atmospheric Cherenkov telescope. We report the results of the observations of H 2356-309, PKS 2155-304, PKS 0537-441, and 3C 279, performed from 2005 to 2009, applying a new analysis to suppress the effects of the position dependence of Cherenkov images in the field of view. No significant VHE gamma ray emission was detected from any of the four blazars. The GeV gamma-ray spectra of these objects were obtained by analyzing Fermi/LAT archival data. Wide range (radio to VHE gamma-ray bands) spectral energy distributions (SEDs) including CANGAROO-III upper limits, GeV gamma-ray spectra, and archival data, even though they are non-simultaneous, are discussed using a one-zone synchrotron self-Compton (SSC) model in combination with a external Compton (EC) radiation. The HBLs (H 2356-309 and PKS 2155-304) can be explained by a simple SSC model, and PKS 0537-441 and 3C 279 are well modeled by a combination of SSC and EC model. We find a consistency with the blazar sequence in terms of strength of magnetic field and component size. 相似文献
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消光法反演腾格里沙漠地区沙尘气溶胶谱分布 总被引:10,自引:5,他引:5
对腾格里沙漠4~9月份的整层大气气溶胶的光学遥感观测结果进行了分析。结果表明,由于消光因子对大粒径粒子消光效应的不敏感性,决定了消光法仅可较好地反演粒径在0.1~5μm之间的气溶胶谱分布特征,特别是对0.1~1μm的大粒子谱分布的反演结果更为稳定;腾格里沙漠气溶胶粒度谱分布基本符合Junge谱;浮尘天气的谱分布同干洁晴好天气的谱分布有着很大的差异,浮尘天气下粒径在0.1~1.0μm的大粒子以及粒径>1.0μm的巨粒子数有明显的增加,浓度要比干洁天气下的大几个量级。在干洁晴好天气下,腾格里沙漠的气溶胶是均一的、稳定的,而且>1μm的大粒子浓度很小;气溶胶的谱分布几乎是一致的,谱形大致为Junge谱,在粒度0.4~1.0μm范围内有一明显峰值。 相似文献
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西北地区东部冰雹云的卫星光谱特征和遥感监测模型 总被引:11,自引:0,他引:11
根据气象台站的冰雹观测记录,针对冰雹灾害多发的西北地区东部,选取2001—2004年间14次NOAA卫星过境的AVHRR资料,共88个样本数,对冰雹云和其他云的光谱特征进行对比分析。结果表明,雹云的热红外亮度温度的变化基本在245K以下,中红外波段反射率相对较低,基本变化在0.4及以下范围,可见光和近红外波段反射率>0.6。冰雹产生的两个重要条件是高的云光学厚度和大的云粒子有效半径共同发生的区域;西北地区冰雹发生的云顶高度基本在4.5~7km之间。根据雹云的光谱特征,确定雹暴指数及其模型阈值>0.35的冰雹监测方法,多普勒雷达回波和气象站观测结果说明,雹暴指数等多参数结合判别冰雹云效果显著。 相似文献
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Long‐term variations and temporal scaling of hydroclimatic time series with focus on the German part of the Elbe River Basin
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Long‐term variations and temporal scaling of mean monthly time series of river flow, precipitation, temperature, relative humidity, air pressure, duration of bright sunshine, degree of cloud cover, short wave radiation, wind speed and potential evaporation within or in vicinity of the German part of the Elbe River Basin are analyzed. Statistically significant correlations between the 2–15 year scale‐averaged wavelet spectra of the hydroclimatic variables and the North Atlantic Oscillation‐ and Arctic Oscillation index are found which suggests that such long‐term patterns in hydroclimatic time series are externally forced. The Hurst parameter estimates (H) based on the Detrended Fluctuation Analysis (DFA) indicate persistence for discharge, precipitation, wind speed, air pressure and the degree of cloud cover, all having an annual cycle and a broad low‐frequency distribution. Also, DFA H parameter estimates are higher for discharge than for precipitation. The major long‐term quasi‐periodic variability modes of precipitation detected using Singular Spectrum Analysis coincide with those detected in the discharge time series. Upon subtraction of these low‐frequency quasi‐periodic modes, the DFA H parameter estimates suggest absence of the persistence for both precipitation and discharge. Copyright © 2013 John Wiley & Sons, Ltd. 相似文献
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P. Felenbok J. Guérin A. Fernandez V. Cayatte C. Balkowski R.C. Kraan-Korteweg 《Experimental Astronomy》1997,7(2):65-85
We are describing a new multi-fibre positioner, MEFOS, that was in generaluse at the La Silla Observatory, and implemented at the prime focus of theESO 3.6 m telescope. It is an arm positioner using 29 arms in a one degreefield. Each arm is equipped with an individual viewing system for accuratesetting and carries two spectroscopic fibres, one for the astronomical objectand the other one for the sky recording needed for sky subtraction. Thespectral fibres intercept 2.5 arcsec on the sky and run from the prime focusto the Cassegrain, where the B&C spectrograph is located. Afterdescribing the observational procedure, we present the first scientificresults. 相似文献
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In an attempt to elucidate the mechanics of deep-water wave breaking, a variety of breaking waves, including spilling and plunging waves, of different length scales and geometries was studied. The waves were generated through wave-wave interactions using wave packets with constant-steepness components, constant-amplitude components, and also components following the Pierson-Moskowitz distribution. Wave steepening prior to breaking were found to cause an increase in the high frequency spectral slope of the wave spectrum. The slopes were correlated to the type of breaking and the intensity of the breaking. The energy loss through breaking varied with the spectral characteristics of the wave packet. On the other hand, it was also noted that, irrespective of the wave packet, the losses were from the higher frequency end of the first harmonics. 相似文献
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井下地震计波形记录的P波垂向分量存在频谱极小(spectrum null)现象,导致接收函数的结果不稳定.本文以首都圈地区为例,基于平面波入射的传播矩阵理论,发展了用于计算井下地震计的接收函数正演方法.在此基础上,分析了井下地震计波形垂向分量频谱极小现象,研究其对接收函数稳定性的影响.结果表明,井下地震计波形记录垂向分量的频谱极小开始出现的频率和地震计的埋深相关.该现象可造成反卷积提取的接收函数不稳定,且不稳定情况出现在频谱极小附近的频段,可通过选择合适的高斯因子压制其对接收函数的影响. 相似文献