Zobrazeno 1 - 10
of 448
pro vyhledávání: '"gao, Yuhang"'
Autor:
Lim, Daye, Van Doorsselaere, Tom, Nakariakov, Valery M., Kolotkov, Dmitrii Y., Gao, Yuhang, Berghmans, David
Publikováno v:
A&A 690, L8 (2024)
Context. Recent observations of decayless transverse oscillations have shown two branches in the relationship between periods and loop lengths. One is a linear relationship, interpreted as a standing mode. The other shows almost no correlation and ha
Externí odkaz:
http://arxiv.org/abs/2409.12095
The investigation into the pairing phase transition in the odd-A nucleus 161Dy utilizes a sophisticated blend of covariant density functional theory and the shell-model-like approach. It is discerned that variations in thermodynamic quantities at the
Externí odkaz:
http://arxiv.org/abs/2408.00423
Publikováno v:
A&A 689, A195 (2024)
Context. In the coronal open-field regions, such as coronal holes, there are many transverse waves propagating along magnetic flux tubes, generally interpreted as kink waves. Previous studies have highlighted their potential in coronal heating, solar
Externí odkaz:
http://arxiv.org/abs/2406.19474
Autor:
Li, Hanlong, Wang, Pei, Wu, Yuhan, Ren, Jing, Gao, Yuhang, Zhang, Lingyun, Zhang, Mingtai, Chen, Wenxin
Wood-leaf classification is an essential and fundamental prerequisite in the analysis and estimation of forest attributes from terrestrial laser scanning (TLS) point clouds,including critical measurements such as diameter at breast height(DBH),above-
Externí odkaz:
http://arxiv.org/abs/2405.18737
Recent observations have revealed two types of decayless transverse oscillations in short coronalloops: one with short periods scaling with loop lengths, and the other with longer periods that exhibit a peak at around 5 min in the period distribution
Externí odkaz:
http://arxiv.org/abs/2308.13813
Autor:
Guo, Jinhan, Qiu, Ye, Ni, Yiwei, Guo, Yang, Li, Chuan, Gao, Yuhang, Schmieder, Brigitte, Poedts, Stefaan, Chen, Pengfei
Solar filaments often exhibit rotation and deflection during eruptions, which would significantly affect the geoeffectiveness of the corresponding coronal mass ejections (CMEs). Therefore, understanding the mechanisms that lead to such rotation and l
Externí odkaz:
http://arxiv.org/abs/2308.08831
Autor:
Guo, Mingzhe, Duckenfield, Timothy, Van Doorsselaere, Tom, Karampelas, Konstantinos, Pelouze, Gabriel, gao, Yuhang
We model a coronal loop as a three-dimensional magnetic cylinder in a realistic solar atmosphere that extends from the chromosphere to the corona. Kink oscillations, believed ubiquitous in the solar corona, are launched in the loop. Heating is expect
Externí odkaz:
http://arxiv.org/abs/2305.03621
Alfv\'enic motions are ubiquitous in the solar atmosphere and their observed properties are closely linked to those of photospheric p-modes. However, it is still unclear how a predominantly acoustic wave driver can produce these transverse oscillatio
Externí odkaz:
http://arxiv.org/abs/2304.01606
The hot nucleus $^{162}\mathrm{Dy}$ is investigated using covariant density functional theory, where the shell-model-like approach treats the pairing correlation. Lee-Yang's theorem is applied to classify the pairing phase transition by analyzing the
Externí odkaz:
http://arxiv.org/abs/2303.09039
The propagation direction and true velocity of a solar coronal mass ejection, which are among the most decisive factors for its geo-effectiveness, are difficult to determine through single-perspective imaging observations. Here we show that Sun-as-a-
Externí odkaz:
http://arxiv.org/abs/2204.11722