output
20052026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations

Showing astro-ph.SRShow all

41 papers · 1 filter

astro-ph.SR2026

Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter

Xiaohang Chen, Gang Li, Joe Giacalone +12

The propagation of solar energetic particles (SEPs) through the heliosphere is primarily guided by the interplanetary magnetic field (IMF) which is embedded in the solar wind plasm…

astro-ph.SR2026★ 1 cited

Statistics of blob properties in two types of coronal streamers

Haiyi Li, Zhenghua Huang, Maria S. Madjarska +4

Previous studies have shown that a streamer blob might originate in the lower corona and thus be affected by activity in that region. While the base of one streamer might differ fr…

astro-ph.SR2025★ 1 cited

Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configuration

Yuwei Li, J. H. Guo, Y. W. Ni +2

Context. Mounting evidence has shown that EUV waves consist of a fast-mode magnetohydrodynamic (MHD) wave (or shock wave) followed by a slower nonwave component, as predicted by th…

astro-ph.SR2023★ 6 cited

TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet

Chen Jiang, Tao Wu, Adina D. Feinstein +30

The Transiting Exoplanet Survey Satellite (TESS) mission searches for new exoplanets. The observing strategy of TESS results in high-precision photometry of millions of stars acros…

astro-ph.SR2022★ 14 cited

First report of a solar energetic particle event observed by China's Tianwen-1 mission in transit to Mars

Shuai Fu, Zheyi Ding, Yongjie Zhang +15

Solar energetic particles (SEPs) associated with flares and/or coronal mass ejection (CME)-driven shocks can impose acute radiation hazards to space explorations. To measure energe…

astro-ph.SR2022★ 2 cited

Existence of The Closed Magnetic Field Lines Crossing The Coronal Hole Boundaries

Guan-Han Huang, Chia-Hsien Lin, Lou-Chuang Lee

Coronal holes (CHs) are regions with unbalanced magnetic flux, and have been associated with open magnetic field (OMF) structures. However, it has been reported that some CHs do no…