Results 1 to 10 of about 4,125 (210)
Proceedings of the International Astronomical Union, 2008 AbstractSolar filaments (or prominences) are magnetic structures in the corona. They can be represented by twisted flux ropes in a bipolar magnetic environment. In such models, the dipped field lines of the flux rope carry the filament material and parasitic polarities in the filament channel are responsible for the existence of the lateral feet of ...
B. Schmieder, G. Aulanier, Tibor Török
openalex +3 more sources
Solar Prominence Interactions [PDF]
The Astrophysical Journal, 2005 We report numerical simulations of the formation, interaction, and magnetic reconnection between pairs of solar prominences within the sheared-arcade model. Our experiments consider the four possible basic combinations of chiralities (identical or opposite) and axial magnetic fields (aligned or opposed) between the participating prominences.
C. R. DeVore +2 more
openalex +4 more sources
Hot prominence spicules launched from turbulent cool solar prominences [PDF]
Astronomy & Astrophysics, 2019 A solar filament is a dense cool condensation that is supported and thermally insulated by magnetic fields in the rarefied hot corona. Its evolution and stability, leading to either an eruption or disappearance, depend on its coupling with the surrounding hot corona through a thin transition region, where the temperature steeply rises.
L. P. Chitta, H. Peter, L. Li
openalex +4 more sources
Nature, 1870 IT may interest some of your readers to hear that the bright lines of the hydrogen “flames” extending beyond the sun's disc can be seen with much less instrumental aid than has hitherto been considered indispensable. I have succeeded in seeing them quite unmistakably by the following very simple means. I fixed one of Mr.
ERNEST CARPMAEL
openalex +2 more sources
Solar Prominences: Observations [PDF]
Living Reviews in Solar Physics, 2014 Solar prominences are one of the most common features of the solar atmosphere. They are found in the corona but they are one hundred times cooler and denser than the coronal material, indicating that they are thermally and pressure isolated from the ...
Susanna Parenti
doaj +2 more sources
Apparent Solar Tornado-Like Prominences [PDF]
Solar Physics, 2013 accepted for publication in Solar Physics (in press)
O. Panasenco, Sara Martin, M. Velli
openalex +4 more sources
Journal of Space Weather and Space Climate, 2023 The Madrid Astronomical Observatory implemented a solar observation program from 1876 to 1986. In addition to sunspots, the observers at this observatory recorded other solar features such as prominences.
Aparicio Alejandro Jesús Pérez +3 more
doaj +1 more source
Solar prominence polarimetry [PDF]
Astronomy & Astrophysics, 2003 We measure the resonance polarization in solar prominences in H α , H β and HeD 3 . A two-dimensional set-up with narrow-band filter, polarization analyzer and CCD camera is used to take prominence images in polarized light at high spatial resolution.
Wiehr, E., Bianda, M.
openaire +2 more sources