Distributed Data-Processing Pipeline for Mingantu Ultrawide Spectral Radioheliograph
文献类型:期刊论文
作者 | Wang F(王锋)1,2,3![]() ![]() ![]() ![]() ![]() ![]() |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
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出版日期 | 2015-04 |
卷号 | 127期号:950页码:383-396 |
ISSN号 | 0004-6280 |
产权排序 | 第三完成单位 |
通讯作者 | Wang, F (reprint author), Kunming Univ Sci & Technol, Comp Technol Applicat Key Lab Yunnan Prov, Chenggong 650500, Kunming, Peoples R China. |
英文摘要 | The Mingantu Ultrawide Spectral Radioheliograph (MUSER) is a synthetic-aperture radio interferometer built in Ming'antu, Inner Mongolia, China. As a solar-dedicated interferometric array, the MUSER can produce high-quality radio images in a frequency range of 400 MHz-15 GHz with high temporal, spatial, and spectral resolution. Implementing of the data processing system for the MUSER is a major challenge to performing high-cadence imaging in wideband and obtaining more than two orders of higher multiple frequencies. There is an urgent need to build a pipeline for processing the massive amount of MUSER data generated each day. In this article, we present a high-performance distributed data processing pipeline (DDPP) built on the OpenCluster infrastructure for processing MUSER observational data, including data storage, preprocessing, image reconstruction, deconvolution, archiving, and real-time monitoring. We comprehensively elaborate the system architecture of the pipeline and the implementation of each subsystem. The DDPP is automatic, robust, scalable, and manageable. The processing performance under a parallel CPU/GPU hybrid system meets the requirements of MUSER data processing. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | FASTBIT |
收录类别 | SCI |
原文出处 | http://www.jstor.org/stable/info/10.1086/680852 |
语种 | 英语 |
WOS记录号 | WOS:000352231000007 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4265] ![]() |
专题 | 云南天文台_其他 |
作者单位 | 1.Computer Technology Application Key Lab of Yunnan Province, Kunming 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, 4.Chinese National Observatory, Chinese Academy of Sciences, Beijing |
推荐引用方式 GB/T 7714 | Wang F,Mei, Y,Deng, H,et al. Distributed Data-Processing Pipeline for Mingantu Ultrawide Spectral Radioheliograph[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2015,127(950):383-396. |
APA | Wang F.,Mei, Y.,Deng, H.,Wang, W.,Liu, CY.,...&Ji, KF.(2015).Distributed Data-Processing Pipeline for Mingantu Ultrawide Spectral Radioheliograph.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,127(950),383-396. |
MLA | Wang F,et al."Distributed Data-Processing Pipeline for Mingantu Ultrawide Spectral Radioheliograph".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 127.950(2015):383-396. |
入库方式: OAI收割
来源:云南天文台
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