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Sunspot light bridges are known to exhibit a variety of dynamic and persistent phenomena such as surges, small-scale jets etc. in the chromosphere and transition region. While it has generally been proposed that magnetic reconnection is…

太阳与恒星天体物理 · 物理学 2021-01-27 Rohan E. Louis , Julia K. Thalmann

High speed photometry in 2008 shows that the light curve of V842 Cen possesses a coherent modulation at 56.825 s, with sidebands at 56.598 s and 57.054 s. These have appeared since this nova remnant was observed in 2000 and 2002. We deduce…

太阳与恒星天体物理 · 物理学 2009-11-13 P. A. Woudt , B. Warner , J. Osborne , K. Page

An analysis of line-of-sight velocity oscillation in nine solar faculae was undertaken with the aim of studying of phase relations between chromosphere (He i 10830 A line) and photosphere (Si i 10827 A line) five-minute oscillations. We…

太阳与恒星天体物理 · 物理学 2015-05-30 N. I. Kobanov , A. S. Kustov , S. A. Chupin , V. A. Pulyaev

The strongest known correspondence between ALMA 3mm emission and other solar observations is between the H-alpha line width and 3 mm brightness temperature, while the typical 3-5min p-mode oscillations found in many chromospheric…

太阳与恒星天体物理 · 物理学 2023-01-10 Lucas A. Tarr , Adam R. Kobelski , Sarah A. Jaeggli , Momchil Molnar , Gianna Cauzzi , Kevin P. Reardon

Helioseismic and magnetohydrodynamic waves are abundant in and above sunspots. Through cross-correlating oscillation signals in the photosphere observed by the SDO/HMI, we reconstruct how waves propagate away from virtual wave sources…

太阳与恒星天体物理 · 物理学 2015-08-19 Junwei Zhao , Ruizhu Chen , Thomas Hartlep , Alexander G. Kosovichev

We have investigated temporal and spectral properties of a large sample of thermonuclear bursts with oscillations from eight different sources with spin frequencies varying from 270 to 620 Hz. For our sample we chose those bursts, for which…

高能天体物理现象 · 物理学 2017-12-27 Manoneeta Chakraborty , Yunus Emre Bahar , Ersin Göğüş

We analyze the time series of Ca II H-line obtained from Hinode/SOT on the solar limb. We follow three cases of upwardly propagating kink waves along a spicule and inverted Y-shaped structures at the cusp of it. The time-distance analysis…

太阳与恒星天体物理 · 物理学 2015-06-22 H. Ebadi , M. Ghiassi

Emerging flux regions (EFRs) are known to exhibit various sporadic local heating events in the lower atmosphere. To investigate the characteristics of these events, especially to link the photospheric magnetic fields and atmospheric…

太阳与恒星天体物理 · 物理学 2017-02-15 Shin Toriumi , Yukio Katsukawa , Mark C. M. Cheung

The presence of intense magnetic fields in and around sunspots is expected to modify the solar structure and oscillation frequencies. Applying the ring diagram technique to data from the Michelson Doppler Imager (MDI) on board the Solar and…

天体物理学 · 物理学 2009-11-07 S. P. Rajaguru , Sarbani Basu , H. M. Antia

Since their discovery, spicules have attracted increased attention as energy/mass bridges between the dense and dynamic photosphere and the tenuous hot solar corona. Mechanical energy of photospheric random and coherent motions can be…

太阳与恒星天体物理 · 物理学 2015-05-13 T. V. Zaqarashvili , R. Erdelyi

Dynamical jets are generally found on Light bridges (LBs), which are key to studying sunspots decays. So far, their formation mechanism is not fully understood. In this paper, we used state-of-the-art observations from the Goode Solar…

太阳与恒星天体物理 · 物理学 2019-01-16 Xianyong Bai , Hector Socas-Navarro , Daniel Nóbrega-Siverio , Jiangtao Su , Yuanyong Deng , Dong Li , Wenda Cao , Kaifan Ji

There are two goals in this study. One is to investigate how frequently white-light flares (WLFs) occur in a flare-productive active region (NOAA active region 11515). The other is to investigate the relationship between WLFs and magnetic…

太阳与恒星天体物理 · 物理学 2018-06-06 Y. L. Song , H. Tian , M. Zhang , M. D. Ding

Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination due to their thread-like features and dynamic behaviors. Utilizing data from the New Vacuum Solar Telescope (NVST), Chinese H_alpha Solar Explorer…

太阳与恒星天体物理 · 物理学 2024-04-05 Jincheng Wang , Dong Li , Chuan Li , Yijun Hou , Zhike Xue , Zhe Xu , Liheng Yang , Qiaoling Li

Aims. Combining high-resolution and synoptic observations aims to provide a comprehensive description of flux emergence at photospheric level and of the growth process that eventually leads to a mature active region. Methods. Small active…

Fibrils in the solar chromosphere carry transverse oscillations as determined from non-spectroscopic imaging data. They are estimated to carry an energy flux of several $\mathrm{kW~m}^{-2}$, which is a significant fraction of the average…

Solar Active Region (AR) 12673 is the most flare productive AR in the solar cycle 24. It produced four X-class flares including the X9.3 flare on 06 September 2017 and the X8.2 limb event on 10 September. Sun and Norton (2017) reported that…

太阳与恒星天体物理 · 物理学 2018-01-10 Haimin Wang , Vasyl Yurchyshyn , Chang Liu , Kwangsu Ahn , Shin Toriumi , Wenda Cao

We present time-series photometry during eruption of the extremely fast nova V1674 Herculis (Nova Her 2021). The 2021 light curve showed periodic signals at 0.152921(3) d and 501.486(5) s, which we interpret as respectively the orbital and…

Light crossing dark domain walls that source a top form coupled to gauge Chern--Simons terms mixing visible and dark $U(1)$ gauge fields generically converts into dark photons. The effect is entirely localized on the wall and requires no…

宇宙学与河外天体物理 · 物理学 2026-02-27 Nemanja Kaloper

Differences between observed and theoretical eigenfrequencies of the Sun have characteristics which identify them as arising predominantly from properties of the oscillations in the vicinity of the solar surface: in the super-adiabatic,…

天体物理学 · 物理学 2007-05-23 C. S. Rosenthal , J. Christensen-Dalsgaard , A. Nordlund , R. F. Stein , R. Trampedach

A critical review of experimental studies of the so-called 'slow light' arising due to anomalously high steepness of the refractive index dispersion under conditions of electromagnetically induced transparency or coherent population…

光学 · 物理学 2009-11-11 E. B. Aleksandrov , V. S. Zapasskii