Results 1 to 10 of about 1,041,175 (227)

Horizontal flow below solar filaments

open access: yesAstronomy and Astrophysics, 2018
Context. Observations of the internal fine structures of solar filaments indicate that the threads of filaments follow magnetic field lines. The magnetic field inside the filament has a strong axial component.
Pavel Ambroz, Werner Pötzi
exaly   +2 more sources

Differential rotation of short-lived solar filaments [PDF]

open access: yesSolar Physics, 1977
We have measured the rotation rate of short-lived solar filaments as a function of their latitude. The resulting rotation curve appears to be somewhat flatter than the corresponding curve for long-lived ...
Tang, Frances, Adams, W. M.
exaly   +1 more source
Some of the next articles are maybe not open access.

Proper motion of solar filaments

Astronomy and Astrophysics, 2002
Pavel Ambroz
exaly  

Proper Motion of Solar Filaments [PDF]

open access: yesAstronomy & Astrophysics, 1999
Precise measurements of heliographic position of solar filaments were used for describing the proper motion of solar filaments on the time-scale of one day. Only the velocity values more accurate than 100 m s−1 were used for the study. The filaments have a tendency to make a shaking or waving of the external structure and also to make a general ...
P. Ambrož, A. Schroll
openaire   +3 more sources

Where Do Solar Filaments Form? [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
AbstractIn the present study, we consider where large, stable solar filaments form relative to underlying magnetic polarities. We find that 92% of all large stable filaments form in magnetic configurations involving the interaction of two or more bipoles. Only 7% form above the Polarity Inversion Line (PIL) of a single bipole. This indicates that a key
Mackay, Duncan H.   +2 more
openaire   +3 more sources

CHIRALITY AND MAGNETIC CONFIGURATIONS OF SOLAR FILAMENTS [PDF]

open access: yesThe Astrophysical Journal, 2017
ABSTRACT It has been revealed that the magnetic topology in the solar atmosphere displays hemispheric preference, i.e., helicity is mainly negative/positive in the northern/southern hemispheres, respectively. However, the strength of the hemispheric rule and its cyclic variation are controversial.
Y. Ouyang (欧阳雨)   +3 more
openaire   +3 more sources

The Connection Between Solar Coronal Cavities And Solar Filaments

open access: yes, 2017
This project has been supported by funding from the Division of Advanced Cyberinfrastructure within the Directorate for Computer and Information Science and Engineering, the Division of As- tronomical Sciences within the Directorate for Mathematical and Physical Sciences, and the Division of Atmospheric and Geospace Sciences within the Directorate for ...
Zawadzki, Brianna (5588942)   +1 more
openaire   +3 more sources

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