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国家重点基础研究发展计划(MOST2011CB811401)

作品数:2 被引量:1H指数:1
发文基金:国家自然科学基金国家重点基础研究发展计划更多>>
相关领域:天文地球电子电信更多>>

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Analysis of the CME-driven shock from the SEP event that occurred on 2006 December 14
2012年
In a solar flare or coronal mass ejection (CME), observations of the subse- quent interplanetary shock provide us with strong evidence of particle acceleration to energies of multiple MeV, even up to GeV. Diffusive shock acceleration is an efficient mechanism for particle acceleration. For investigating the shock structure, the energy injection and energy spectrum ofa CME-driven shock, we perform a dynamical Monte Carlo simulation of the CME-driven shock that occurred on 2006 December 14 using an anisotropic scattering law. The simulated results of the shock's fine structure, par- ticle injection, and energy spectrum are presented. We find that our simulation results give a good fit to the observations from multiple spacecraft.
Xin WangYi-Hua Yan
第3章 太阳射电频谱成像观测
<正>在厘米和分米波段的频谱成像对于研究能量释放、粒子加速和粒子输运等基本问题具有重要意义,该波段对应着耀斑初始能量释放区域。未来以中国射电日像仪为代表的新的主要观测设施将在宽频带区域获得高空间分辨率和高动态范围射电图像...
颜毅华
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Antenna system characteristics and solar radio burst observations被引量:1
2015年
The Chinese Spectral Radio Heliograph(CSRH) is an advanced aperture synthesis solar radio heliograph, independently developed by National Astronomical Observatories, Chinese Academy of Sciences. It consists of 100 reflector antennas,which are grouped into two antenna arrays(CSRH-I and CSRH-II) for low and high frequency bands respectively. The frequency band of CSRH-I is 0.4–2 GHz and that for CSRH-II is 2–15 GHz. In the antenna and feed system, CSRH uses eleven feeds to receive signals coming from the Sun. The radiation pattern has a lower side lobe and the back lobe of the feed is well illuminated. The characteristics of gain G and antenna noise temperature T affect the quality of solar radio imaging. For CSRH, the measured G is larger than 60 d Bi and T is less than 120 K. After CSRH-I was established, we successfully captured a solar radio burst between 1.2–1.6 GHz on 2010 November12 using this instrument and this event was confirmed through observations with the Solar Broadband Radio Spectrometer at 2.84 GHz and the Geostationary Operational Environmental Satellite. In addition, an image obtained from CSRH-I clearly revealed the profile of the solar radio burst. The other observational work involved the imaging the Fengyun-2E geosynchronous satellite which is assumed to be a point source.Results indicate that the data processing method applied in this study for deleting errors in a noisy image could be used for processing images from other sources.
Sha LiYi-Hua YanZhi-Jun ChenWei WangDong-Hao Liu
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