output
20202022
most citedSome interesting topics provoked by the solar filament research in the past decade

78 citations

26 papers

astro-ph.EP2022★ 4 cited

Mid-IR Observations of IRAS, AKARI, WISE/NEOWISE and Subaru for Large Icy Asteroid (704) Interamnia: a New Perspective of Regolith Properties and Water Ice Fraction

Haoxuan Jiang, Jianghui Ji, Liangliang Yu +3

(704) Interamnia is one of the largest asteroids that locates in the outer main-belt region, which may contain a large amount of water ice underneath its surface. We observe this a…

hep-ph2022★ 2 cited

Dineutron decay into sterile anti-neutrinos in neutron stars and its observable consequences

Yongliang Hao, Dongdong Ni

In some extensions of the Standard Model (SM), two neutrons are allowed to decay into two sterile anti-neutrinos () via new scalar bosons. This process v…

astro-ph.EP2022★ 11 cited

Boundary Layers of Circumplanetary Disks around Spinning Planets I. Effects of Rossby Waves

Zhihao Fu, Shunquan Huang, Cong Yu

Gas giant planets are believed to accrete from their circumplanetary disks (CPDs). The CPDs usually involve accretion through the boundary layer (BL) in the vicinity of planets. Pr…

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…

astro-ph.SR2022★ 1 cited

LAMOST MRS-N Observations of the W80 Region

Yao Li, Chao-Jian Wu, Yong-Qiang Yao +12

The spectral observations and analysis for the W80 Region are presented by using the data of Medium-Resolution Spectroscopic Survey of Nebulae (MRS-N) with the Large Sky Area Multi…

astro-ph.EP2022★ 17 cited

Rossby Wave Instabilities of Protoplanetary Discs with Cooling

Shunquan Huang, Cong Yu

Rossby wave instabilities (RWIs) usually lead to nonaxisymmetric vortices in protoplanetary discs and some observed sub-structures of these discs can be well explained by RWIs. We…