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Solar Ultraviolet Bursts

by Katsukawa, Yukio , Peter, Hardi , Berlicki, Arkadiusz , Madjarska, Maria S. , Vissers, Gregal J. M. , Cheung, Mark C. M. , Madsen, Chad , Rutten, Robert J. , Huang, Zhenghua , Schmieder, Brigitte , Reardon, Kevin P. , Heinzel, Petr , Nelson, Chris J. , Danilovic, Sanja , Tian, Hui , Chitta, L. P. , Toriumi, Shin , van der Voort, Luc H. M. Rouppe , Young, Peter R.

in Aerospace Technology and Astronautics / Astrophysics / Astrophysics and Astroparticles / Atmosphere / Bombs / Bursting / Bursts / Diagnostic systems / Ellerman bombs / Magnetic flux / Magnetic reconnection / Observatories / Photosphere / Physics / Physics and Astronomy / Planetology / Polarity / Science / Solar activity / Solar activity regions / Solar atmosphere / Solar corona / Solar physics / Space Exploration and Astronautics / Space science / Space Sciences (including Extraterrestrial Physics / Spectrometry / Sun / Sun: activity / Sun: atmosphere / Sun: transition region / Sun: UV radiation / Sunspots / Ultraviolet astronomy / Wavelengths

2018

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2018

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2018

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Journal Article

Solar Ultraviolet Bursts

Katsukawa, Yukio,

Peter, Hardi,

Berlicki, Arkadiusz,

Madjarska, Maria S.,

Vissers, Gregal J. M.,

Cheung, Mark C. M.,

Madsen, Chad,

Rutten, Robert J.,

Huang, Zhenghua,

Schmieder, Brigitte,

Reardon, Kevin P.,

Heinzel, Petr,

Nelson, Chris J.,

Danilovic, Sanja,

Tian, Hui,

Chitta, L. P.,

Toriumi, Shin,

van der Voort, Luc H. M. Rouppe,

Young, Peter R.

2018

Overview

The term “ultraviolet (UV) burst” is introduced to describe small, intense, transient brightenings in ultraviolet images of solar active regions. We inventorize their properties and provide a definition based on image sequences in transition-region lines. Coronal signatures are rare, and most bursts are associated with small-scale, canceling opposite-polarity fields in the photosphere that occur in emerging flux regions, moving magnetic features in sunspot moats, and sunspot light bridges. We also compare UV bursts with similar transition-region phenomena found previously in solar ultraviolet spectrometry and with similar phenomena at optical wavelengths, in particular Ellerman bombs. Akin to the latter, UV bursts are probably small-scale magnetic reconnection events occurring in the low atmosphere, at photospheric and/or chromospheric heights. Their intense emission in lines with optically thin formation gives unique diagnostic opportunities for studying the physics of magnetic reconnection in the low solar atmosphere. This paper is a review report from an International Space Science Institute team that met in 2016–2017.

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Publisher

Springer Netherlands,Springer Nature B.V,Springer Verlag

Subject

Aerospace Technology and Astronautics

/ Astrophysics

/ Astrophysics and Astroparticles

/ Atmosphere

/ Bombs

/ Bursting

/ Bursts