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Two Quasi-periodic Oscillations in ESO 113-G010
DOI: 10.1016/j.chinastron.2020.04.002 Bibcode: 2020ChA&A..44...32Z

Zhang, Peng; Yan, Jing-Zhi; Liu, Qing-Zhong

In the narrow-line Seyfert galaxy (NLS1) ESO 113-G010, two quasi-periodic oscillation (QPO) signals are detected in the XMM-Newton data collected in 2005 November. The XMM-Newton telescope has an exposure longer than 100 ks in the energy range of 0.3-10 keV. The data are analyzed using the Lomb-Scargle periodogram (LSP) and the weighted wavelet Z-…

2020 Chinese Astronomy and Astrophysics
XMM-Newton 6
Automatic Coronagraph Image Classification with Machine Learning Methods
DOI: 10.1016/j.chinastron.2020.11.006 Bibcode: 2020ChA&A..44..507S

Zhang, Yan; Feng, Li; Li, Hui +5 more

The detection of Coronal Mass Ejections (CMEs) is an important prerequisite for establishing a CME event database and realizing the prediction of CME interplanetary propagation. The Lyman-alpha Solar Telescope (LST) aboard the ASO-S (Advanced Space-based Solar Observatory) satellite will be equipped with a white-light coronagraph. The images with …

2020 Chinese Astronomy and Astrophysics
SOHO 6
Study of the Streamer Current Sheet with White-Light and UV Observations
DOI: 10.1016/j.chinastron.2020.11.004 Bibcode: 2020ChA&A..44..474S

Feng, Li; Li, Hui; Shi, Guang-lu +2 more

Current sheets (CSs) are the main region where magnetic reconnections can convert magnetic energy into plasma thermal and kinetic energies. We have studied a CS in the streamer occurred on 3 January 2003 by combining the White-Light (WL) images observed by the Large Angle and Spectrometric Coronagraph (LASCO) and the EUV spectra detected by the Ul…

2020 Chinese Astronomy and Astrophysics
SOHO 2
The Galactic Aberration and Its Impact on Astronomical Reference Frames
DOI: 10.1016/j.chinastron.2020.05.001 Bibcode: 2020ChA&A..44..131L

Liu, Jia-cheng; Liu, Niu

The Galactic aberration effect, also known as the secular aberration drift, is a consequence of the centripetal acceleration of the Solar System Barycenter in the circular orbit around the Galactic center. It causes distance-independent apparent proper motions (the amplitude is about 5 µas · yr - 1) for extragalactic sources which…

2020 Chinese Astronomy and Astrophysics
Gaia 1