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相关论文: Spectroscopic evidence for helicity in explosive e…

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In this paper, we extend our earlier work to provide additional evidence for an alternative scenario to explain the nature of so-called `explosive events'. The bi-directed, fast Doppler motion of explosive events observed spectroscopically…

太阳与恒星天体物理 · 物理学 2015-06-03 W. Curdt , H. Tian , S. Kamio

Explosive events are small transition region phenomena characterised by broad non-Gaussian wings in their line profiles. Images from the Solar Dynamics Observatory (SDO) give a first view of the plasma dynamics at the sites of explosive…

太阳与恒星天体物理 · 物理学 2015-06-11 Davina Innes , Luca Teriaca

We investigate high resolution spectroscopic and imaging observations from the CRisp Imaging SpectroPolarimeter (CRISP) instrument to study the dynamics of chromospheric spicule type events. It is widely accepted that chromospheric fine…

太阳与恒星天体物理 · 物理学 2021-12-30 Juie Shetye , Erwin Verwichte , Marco Stangalini , J. G. Doyle

Spicules are among the most ubiquitous small-scale, jet-like features in the solar chromosphere and are widely believed to play a significant role in transporting mass and energy into the solar corona with their mechanisms not fully…

太阳与恒星天体物理 · 物理学 2025-12-09 Jeongwoo Lee , Eun-Kyung Lim , Viggo Hansteen

We performed a 3D radiative MHD simulation of the solar atmosphere. This simulation shows a jet-like feature that shows similarities to the type II spicules observed for the first time with Hinode. Rapid Blueshifted Events (RBEs) on the…

Over the last two decades the uninterrupted, high-resolution observations of the Sun, from the excellent range of telescopes aboard many spacecraft complemented with observations from sophisticated ground-based telescopes have opened up a…

太阳与恒星天体物理 · 物理学 2015-06-05 G. Tsiropoula , K. Tziotziou , I. Kontogiannis , M. S. Madjarska , J. G. Doyle , Y. Suematsu

Spicules are the most ubuiquitous type of jets in the solar atmosphere. The advent of high-resolution imaging and spectroscopy from the Interface Region Imaging Spectrograph (IRIS) and ground-based observatories has revealed the presence of…

太阳与恒星天体物理 · 物理学 2017-11-01 Bart De Pontieu , Juan Martinez-Sykora , Georgios Chintzoglou

New instrumental and telescopes covering the optical and ultra-violet spectral regions have revealed a range of small-scale dynamic features, many which may be related. For example, the range of spicule-like features hints towards a…

太阳与恒星天体物理 · 物理学 2023-08-02 Nived Vilangot Nhalil , Juie Shetye , J. Gerry Doyle

Chromospheric observations taken at high cadence and high spatial resolution show a range of spicule like features, including Type I, Type II (as well as RBEs and RREs) and those which seem to appear within a few seconds, which if…

太阳与恒星天体物理 · 物理学 2016-04-20 J. Shetye , J. G. Doyle , E. Scullion , C. J. Nelson , D. Kuridze , V. Henriques , F. Woeger , T. Ray

Bunches of swaying and spinning plasma jets in the solar atmosphere - the spicules - exhibit a variety of complex dynamics that are clearly observed in the images of the solar limb. Utilizing three-dimensional radiative magnetohydrodynamics…

太阳与恒星天体物理 · 物理学 2024-04-26 Sahel Dey , Piyali Chatterjee , Robertus Erdelyi

In this research, we investigate Explosive Events (EEs) in the off-limb solar atmosphere, with simultaneous observations from the Si IV, Mg II k, and slit-jaw images (SJI) of the Interface Region Imaging Spectrograph (IRIS), on 17 August…

太阳与恒星天体物理 · 物理学 2022-07-06 E. Tavabi , S. Zeighami , M. Heydari

Spicules are the thin hair/grass-like structures that are prominently observed at the chromospheric solar limb. It is believed that fibrils and rapid blueshifted and redshifted excursions (RBEs and RREs; collectively referred to as REs)…

太阳与恒星天体物理 · 物理学 2024-08-09 Ravi Chaurasiya , Ankala Raja Bayanna , R. E. Louis , T. M. D. Pereira , S. K. Mathew

The solar atmosphere contains a wide variety of small-scale transient features. Here, we explore the inter-relation between some of them such as surges, explosive events and blinkers via simultaneous spectral and imaging data taken with the…

太阳与恒星天体物理 · 物理学 2009-07-24 M. S. Madjarska , J. G. Doyle , B. de Pontieu

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

The Interface Region Imaging Spectrograph (IRIS) of the NASA small explorer mission provides significantly more complete and higher resolution spectral coverage of the dynamical conditions inside the chromosphere and transition region (TR)…

太阳与恒星天体物理 · 物理学 2015-10-28 E. Tavabi , S. Koutchmy , L. Golub

Using high-speed photography, we investigate two distinct regimes of the impact dynamics of granular jets with non-circular cross-sections. In the steady-state regime, we observe the formation of thin granular sheets with anisotropic shapes…

软凝聚态物质 · 物理学 2014-08-26 Xiang Cheng , Leonardo Gordillo , Wendy W. Zhang , Heinrich M. Jaeger , Sidney R. Nagel

Helicity, a measure of the breakage of reflectional symmetry representing the topology of turbulent flows, contributes in a crucial way to their dynamics and to their fundamental statistical properties. We review several of their main…

等离子体物理 · 物理学 2022-02-16 Annick Pouquet , Nobumitsu Yokoi

We present a theoretical and numerical study on the motion of isotropic helicoids in complex flows. These are particles whose motion is invariant under rotations but not under mirror reflections of the particle. This is the simplest, yet…

流体动力学 · 物理学 2016-09-19 Kristian Gustavsson , Luca Biferale

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…

Spicules are ubiquitous, small-scale features in the solar atmosphere, exhibiting a jet-like appearance most clearly identified by their apparent motion in off-limb observations. While they are often interpreted as narrow, thread-like…

太阳与恒星天体物理 · 物理学 2026-05-26 Sanghita Chandra , Robert Cameron , Damien Przybylski , Sami K. Solanki
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