Zobrazeno 1 - 10
of 102
pro vyhledávání: '"WANG Chuanbing"'
Autor:
LIU Zimo, TANG Bin, HUANG Zhihong, WANG Chuanbing, ZHANG Qilin, CHENG Song, CHEN Xuzhi, SUN Changhong
Publikováno v:
Meikuang Anquan, Vol 53, Iss 2, Pp 74-79 (2022)
The pipe jacking method has high construction safety, fast tunneling speed, convenient and flexible construction. However, if it is used in deep strata of coal mines, it will face challenges such as high ground stress and complex geological condition
Externí odkaz:
https://doaj.org/article/17a150a31e0a44c6b615c86caf9681a5
Autor:
Wang Jingjing, Ao Xianzhi, Wang Yuming, Wang Chuanbing, Cai Yanxia, Luo Bingxian, Liu Siqing, Shen Chenglong, Zhuang Bin, Xue Xianghui, Gong Jiancun
Publikováno v:
Journal of Space Weather and Space Climate, Vol 8, p A39 (2018)
We present in this paper an operational solar wind prediction system. The system is an outcome of the collaborative efforts between scientists in research communities and forecasters at Space Environment Prediction Center (SEPC) in China. This system
Externí odkaz:
https://doaj.org/article/b3b053466bf742668cf5db1c39ffb11a
Magnetic reconnection preferentially takes place at the intersection of two separatrices or two quasi-separatrix layers, which can be quantified by the squashing factor Q, whose calculation is computationally expensive due to the need to trace as man
Externí odkaz:
http://arxiv.org/abs/2208.12569
Autor:
Zhang, PeiJin, Zucca, Pietro, Kozarev, Kamen, Carley, Eoin, Wang, ChuanBing, Franzen, Thomas, Dabrowski, Bartosz, Krankowski, Andrzej, Magdalenic, Jasmina, Vocks, Christian
Radio emission of the quiet Sun is considered to be due to thermal bremsstrahlung emission of the hot solar atmosphere. The properties of the quiet Sun in the microwave band have been well studied, and they can be well described by the spectrum of br
Externí odkaz:
http://arxiv.org/abs/2205.00065
To better understand the physical processes associated with Jovian decametric (DAM) radio emissions, we present the statistical study of DAMs and inferred characteristics of DAM sources based on multi-view observation from Wind and STEREO spacecraft.
Externí odkaz:
http://arxiv.org/abs/2201.03148
Recently, we developed the Correlation-Aided Reconstruction (CORAR) method to reconstruct solar wind inhomogeneous structures, or transients, using dual-view white-light images (Li et al. 2020; Li et al. 2018). This method is proved to be useful for
Externí odkaz:
http://arxiv.org/abs/2101.03276
The observed features of the radio sources indicate complex propagation effects embedded in the waves of solar radio bursts. In this work, we perform ray-tracing simulations on radio wave transport in the corona and interplanetary region with anisotr
Externí odkaz:
http://arxiv.org/abs/2101.00911
The radioheliograph image is essential for the study of solar short term activities and long term variations, while the continuity and granularity of radioheliograph data is not so ideal, due to the short visible time of the sun and the complex elect
Externí odkaz:
http://arxiv.org/abs/2006.13023
Autor:
Zhang, PeiJin, Zucca, Pietro, Sridhar, Sarrvesh Seethapuram, Wang, ChuanBing, Morosan, Diana E., Dabrowski, Bartosz, Krankowski, Andrzej, Bisi, Mario M., Magdalenic, Jasmina, Vocks, Christian, Mann, Gottfried
Publikováno v:
A&A 639, A115 (2020)
Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar radio bursts with short time duration may be used as a proxy to underst
Externí odkaz:
http://arxiv.org/abs/2005.09419
Autor:
Zhang, PeiJin, Zucca, Pietro, Wang, ChuanBing, Bisi, Mario M., Dabrowski, Bartosz, Fallows, Richard A., Krankowski, Andrzej, Magdalenic, Jasmina, Mann, Gottfried, Morosan, Diana E., Vocks, Christian
Solar S-bursts are short duration ($<1$ s at decameter wavelengths) radio bursts that have been observed during periods of moderate solar activity, where S stands for short. The frequency drift of S-bursts can reflect the density variation and the mo
Externí odkaz:
http://arxiv.org/abs/2002.02133