Zobrazeno 1 - 10
of 4 699
pro vyhledávání: '"Hong, J. P."'
Autor:
Livernois, A. R., Aros, F. I., Vesperini, E., Askar, A., Bellini, A., Giersz, M., Hong, J., Hypki, A., Libralato, M., Ziliotto, T.
We present the results of Monte Carlo simulations aimed at exploring the evolution towards energy equipartition of first- (1G) and second-generation (2G) stars in multiple-population globular clusters and how this evolution is affected by the initial
Externí odkaz:
http://arxiv.org/abs/2410.12968
Studies on the dynamics of solar filaments have significant implications for understanding their formation, evolution, and eruption, which are of great importance for space weather warning and forecasting. The H$\alpha$ Imaging Spectrograph (HIS) onb
Externí odkaz:
http://arxiv.org/abs/2402.14209
Publikováno v:
International Journal of Nanomedicine, Vol Volume 19, Pp 11941-11956 (2024)
Qingpeng Xie,1,2,* Jiawen Gu,1,2,* Yujia Sun,3 Jinjia Hong,1,2 Jia Wang,1,2 Na Li,1,2 Yuan Zhang,1,2 Meixian Liu,1,2 Xiaoxuan Zhang,1,2 Xiangyu Zhao,1,2 Xiaohang Chen,1,2 Xing Wang1,2 1Shanxi Medical University School and Hospital of Stomatol
Externí odkaz:
https://doaj.org/article/820aa85f02ca425b9c2282d7d2e9363e
Autor:
Bi, Y., Yang, J. J., Qin, Y., Qiang, Z. P., Hong, J. C., Yang, B., Xu, Z., Liu, H., Ji, K. F.
Publikováno v:
A&A 679, A9 (2023)
Nanoflares are impulsive energy releases by magnetic reconnection in the braided coronal magnetic field, which is a potential mechanism for heating the corona. However, there are still sporadic observations of the interchange of braiding structure se
Externí odkaz:
http://arxiv.org/abs/2309.10049
Publikováno v:
A&A 675, A171 (2023)
Context. The Si IV lines at 1394 \r{A} and 1403 \r{A} form in the solar atmosphere at a temperature of $\sim10^{4.8}$ K. They are usually considered optically thin, but their opacity can be enhanced during solar flares. Traditionally, the intensity r
Externí odkaz:
http://arxiv.org/abs/2306.08296
Publikováno v:
Infection and Drug Resistance, Vol Volume 17, Pp 4001-4009 (2024)
Xiang Huo,1 Zhongming Tan,1,2 Huimin Qian,1,2 Yuanfang Qin,1,2 Chen Dong,1,2 Chuchu Li,1,2 Xiaoxiao Kong,1,2 Jie Hong1,2 1National Health Commission (NHC) Key Laboratory of Enteric Pathogenic Microbiology, Jiangsu Provincial Center for Disease Contro
Externí odkaz:
https://doaj.org/article/c7eb66c627244bf4bedefe584dab88fc
Publikováno v:
Cancer Management and Research, Vol Volume 16, Pp 977-988 (2024)
Minmin Shen,1– 3,* Qiaojing Lin,1,2,* Xi Zou,1– 3 Yufan Wu,1,2 Zhihong Lin,1,2 Linglong Shao,1,2 JinSheng Hong,1– 3 Jinmei Chen1– 3 1Department of Radiotherapy, Cancer Center, The First Affiliated Hospital of Fujian Medical University, Fuzhou
Externí odkaz:
https://doaj.org/article/4e0e671710014e18a16cf536c5c3f765
Publikováno v:
Clinical Interventions in Aging, Vol Volume 19, Pp 1203-1215 (2024)
Song Wang,1,* Xiang Zhang,1,* Bo Qu,2,* Kunhai Yang,1 Yongrong Hu,1 Hao Liu,2 Juntao Hong,2 Hao Niu,3 Hongsheng Yang2 1School of Clinical Medicine, Chengdu Medical College, Chengdu, Sichuan, People’s Republic of China; 2Department of Or
Externí odkaz:
https://doaj.org/article/4d3a3811c9944cc1bd51e05025bcfb2d
Publikováno v:
Diabetes, Metabolic Syndrome and Obesity, Vol Volume 17, Pp 2671-2681 (2024)
Jianwen Zhao,1– 5,* Xintian Cai,1– 5,* Junli Hu,1– 5 Shuaiwei Song,1– 5 Qing Zhu,1– 5 Di Shen,1– 5 Wenbo Yang,1– 5 Qin Luo,1– 5 Xiaoguang Yao,1– 5 Delian Zhang,1– 5 Jing Hong,1– 5 Nanfang Li1– 5 1Hypertension Center of
Externí odkaz:
https://doaj.org/article/eba51660fcb046bba475c90298779b6a
Publikováno v:
A&A 668, A96 (2022)
Context. Radiative losses are an indispensable part in the numerical simulation of flares. Detailed calculations could be computationally expensive, especially in the chromosphere. There have been some approximate recipes for chromospheric radiative
Externí odkaz:
http://arxiv.org/abs/2210.04461