A detailed study was made of the lifetimes and evolution of fibrils in McMath 12417, using high resolution filtergrams in H alpha and CaII K made at Big Bear Solar Observatory. It was found that the lifetime of a fibril increases monotonically with its length. This relationship, together with the form of the variation of fibril lengths as a function of time, suggests that fibrils result from material being impulsively injected into magnetic field lines at approximately 30 km/sec, and returning under gravity. The lifetimes and apparent lengths of fibrils are then a function of the inclination of the field lines only. A study of wavelength scans through the H alpha line confirms that the apparent expansion and contraction of fibrils represent...
International audienceContext. The emission of Ca and Hα is correlated for the Sun, but this does no...
In this work, the dynamics of one particular fibril were investigated through high-resolution multi-...
This paper considers the hemispheric pattern of solar filaments using newly developed simulations of...
We present unprecedented high resolution H-alpha observations, obtained with the Swedish 1-m Solar T...
Analysis of sequential H alpha images of active region prominence formation suggests that simple lar...
Aims: We examine the movements of mass elements within dense fibrils using passive tracer particles ...
R. Gafeira et. al.©2017 The American Astronomical Society. All rights reserved. We use seeing-free h...
We use seeing-free high spatial resolution Ca ii H data obtained by the Sunrise observatory to deter...
R. Gafeira et. al.©2017 The American Astronomical Society. All rights reserved. We report the detect...
Current observational instruments are now providing data with the necessary temporal and spatial cad...
Context. Except for the $\ion{Ca}{\sc ii}$ resonance lines, fibrils are ubiquitously present in most...
Fibrils are thin elongated features visible in the solar chromosphere in and around magnetized regio...
We investigate whether flux cancellation is responsible for the formation of a very massive filament...
Aims. We examine the movements of mass elements within dense fibrils using passive tracer particles ...
We consider the physical origin of the hemispheric pattern of filament chirality on the Sun. Our 3D ...
International audienceContext. The emission of Ca and Hα is correlated for the Sun, but this does no...
In this work, the dynamics of one particular fibril were investigated through high-resolution multi-...
This paper considers the hemispheric pattern of solar filaments using newly developed simulations of...
We present unprecedented high resolution H-alpha observations, obtained with the Swedish 1-m Solar T...
Analysis of sequential H alpha images of active region prominence formation suggests that simple lar...
Aims: We examine the movements of mass elements within dense fibrils using passive tracer particles ...
R. Gafeira et. al.©2017 The American Astronomical Society. All rights reserved. We use seeing-free h...
We use seeing-free high spatial resolution Ca ii H data obtained by the Sunrise observatory to deter...
R. Gafeira et. al.©2017 The American Astronomical Society. All rights reserved. We report the detect...
Current observational instruments are now providing data with the necessary temporal and spatial cad...
Context. Except for the $\ion{Ca}{\sc ii}$ resonance lines, fibrils are ubiquitously present in most...
Fibrils are thin elongated features visible in the solar chromosphere in and around magnetized regio...
We investigate whether flux cancellation is responsible for the formation of a very massive filament...
Aims. We examine the movements of mass elements within dense fibrils using passive tracer particles ...
We consider the physical origin of the hemispheric pattern of filament chirality on the Sun. Our 3D ...
International audienceContext. The emission of Ca and Hα is correlated for the Sun, but this does no...
In this work, the dynamics of one particular fibril were investigated through high-resolution multi-...
This paper considers the hemispheric pattern of solar filaments using newly developed simulations of...