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相关论文: Small-Scale Structuring Of Ellerman Bombs at Solar…

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We aim to investigate the temperature enhancements and formation heights of impulsive heating phenomena in solar active-regions such as Ellerman bombs (EBs), ultraviolet bursts (UVBs), and flaring active-region fibrils (FAFs) using…

太阳与恒星天体物理 · 物理学 2020-11-04 J. M. da Silva Santos , J. de la Cruz Rodríguez , S. M. White , J. Leenaarts , G. J. M. Vissers , V. H. Hansteen

Ellerman bombs are transient brightenings of the wings of the solar Balmer lines that mark reconnection in the photosphere. Ellerman noted in 1917 that he did not observe such brightenings in the Na I D and Mg I b lines. This non-visibility…

太阳与恒星天体物理 · 物理学 2016-12-20 R. J. Rutten , L. H. M. Rouppe van der Voort , G. J. M. Vissers

Recent observations from the Interface Region Imaging Spectrograph (IRIS) appear to show impulsive brightenings in high temperature lines, which when combined with simultaneous ground based observations in H$\alpha$, appear co-spatial to…

太阳与恒星天体物理 · 物理学 2017-02-08 A. Reid , M. Mathioudakis , A. Kowalski , J. G. Doyle , J. C. Allred

Burst-like events with signatures in the UV are often observed co-spatial to strong line-of-sight photospheric magnetic fields. Several authors, for example, have noted the spatial relationship between Ellerman bombs (EBs) and Moving…

太阳与恒星天体物理 · 物理学 2016-08-24 C. J. Nelson , J. G. Doyle , R. Erdelyi

We present fast cadence and high resolution observations of flare ribbons from the Solar Orbiter Extreme Ultraviolet Imager (EUI). Utilizing the short-exposure observations from the EUI High Resolution Imager in EUV (HRIEUV), we find…

Small-scale Brightenings (SBs) are commonly observed in the transition region that separates the solar chromosphere from the corona. These brightenings, omnipresent in active region patches known as "moss" regions, could potentially…

Ellerman bombs (EBs) with significant H$\alpha$ wing emissions and ultraviolet bursts (UV bursts) with strong Si IV emissions are two kinds of small transient brightening events that occur in the low solar atmosphere.We numerically…

太阳与恒星天体物理 · 物理学 2024-02-22 Guanchong Cheng , Lei Ni , Yajie Chen , Jun Lin

Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles with enhanced wings at Doppler velocities of 50-150 km/s. They are believed to be the signature of solar phenomena that are one of the main…

太阳与恒星天体物理 · 物理学 2016-11-15 Z. Huang , M. S. Madjarska , E. M. Scullion , L. -D. Xia , J. G. Doyle , T. Ray

Quiet Sun Ellerman Bombs (QSEBs) are key indicators of small-scale photospheric magnetic reconnection events. Recent high-resolution observations have shown that they are ubiquitous and that large numbers of QSEBs can be found in the quiet…

太阳与恒星天体物理 · 物理学 2024-09-11 Aditi Bhatnagar , Luc Rouppe van der Voort , Jayant Joshi

We explore the link between solar energetic particles (SEPs) observed at 1 AU and large-scale disturbances propagating in the solar corona, named after the Extreme ultraviolet Imaging Telescope (EIT) as EIT waves, which trace the lateral…

太阳与恒星天体物理 · 物理学 2015-06-18 R. Miteva , K. -L. Klein , I. Kienreich , M. Temmer , A. Veronig , O. E. Malandraki

In the highly dynamic chromosphere, there exist many kinds of small-scale activities, such as spicules, surges, and Ellerman bombs. Here, we report the discovery of a new phenomenon in the chromosphere observed with the New Vacuum Solar…

太阳与恒星天体物理 · 物理学 2019-08-07 Shuhong Yang , Jun Zhang , Xiaohong Li , Zhong Liu , Yongyuan Xiang

High cadence high spatial resolution observations in H-alpha with the Swedish 1-m Solar Telescope on La Palma have revealed the existence of small-scale highly dynamic bright blobs. A fast wavelength tuning spectro-polarimeter provides…

太阳与恒星天体物理 · 物理学 2015-06-03 Y. Lin , O. Engvold , L. H. M. Rouppe van der Voort

We select and investigate six global solar extreme-ultraviolet (EUV) wave events using data from the Solar Dynamics Observatory and the Solar and Heliospheric Observatory. These eruptions are all on the limb but recorded as halo coronal…

太阳与恒星天体物理 · 物理学 2024-11-19 Huidong Hu , Bei Zhu , Ying D. Liu , Chong Chen , Rui Wang , Xiaowei Zhao

Context. The observation of >100 MeV {\gamma}-rays in the minutes to hours following solar flares suggests that high-energy particles interacting in the solar atmosphere can be stored and/or accelerated for long time periods. The occasions…

太阳与恒星天体物理 · 物理学 2017-12-27 I. Plotnikov , A. P. Rouillard , G. H. Share

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

Quiet-Sun Ellerman bombs (QSEBs) are small-scale magnetic reconnection events in the lower atmosphere of the quiet Sun. Recent work has shown that a small percentage of them can occur co-spatially and co-temporally to ultraviolet (UV)…

太阳与恒星天体物理 · 物理学 2025-01-22 Aditi Bhatnagar , Avijeet Prasad , Luc Rouppe van der Voort , Daniel Nóbrega-Siverio , Jayant Joshi

We revisit the full variety of observed temporal and spatial distributions of energetic solar protons in "gradual" solar energetic-particle (SEP) events resulting from the spatial variations in the shock waves that accelerate them.…

太阳与恒星天体物理 · 物理学 2023-02-16 Donald V. Reames

In this article we present examples of a wider study of space-time correlation of electron precipitation event of the Van Allen belts with the position and time of occurrence of strong (M>6.5) earthquakes. The study is based on the analysis…

地球物理 · 物理学 2010-12-17 G. Anagnostopoulos , V. Rigas , E. Vassiliadis

We have obtained H$\alpha$ high spatial and time resolution observations of the upper solar chromosphere and supplemented these with multi-wavelength observations from the Solar Dynamic Observatory (SDO) and the {\it Hinode}…

太阳与恒星天体物理 · 物理学 2015-05-27 Damian J. Christian , David B. Jess , Patrick Antolin , Mihalis Mathioudakis

Ellerman bombs are bright emission features observed in the wings of H$\alpha$, usually in the vicinity of magnetic concentrations. Here we show that they can also be detected in the Ca II infrared triplet lines, which are easier to…

天体物理学 · 物理学 2009-11-11 H. Socas-Navarro , V. Martinez Pillet , D. Elmore , A. Pietarila , B. W. Lites , R. Manso Sainz