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Publikováno v:
The Astrophysical Journal, Volume 814, Issue 1, article id. 68, 12 pp. (2015)
Knowledge of the electron density distribution in the solar corona put constraints on the magnetic field configurations for coronal modeling and on initial conditions for solar wind modeling. We work with polarized SOHO/LASCO-C2 images from the last
Externí odkaz:
http://arxiv.org/abs/1512.04135
Solar magnetic fields, as well as temperature changes, introduce pressure deviations that play a significant role in modulating the resonant frequencies of p-mode oscillations. Those pressure deviations occurring in the atmosphere or sub-surface of t
Externí odkaz:
https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.720261
Autor:
Maunder, Megan L.1 (AUTHOR) mlm216@exeter.ac.uk, Foullon, Claire1 (AUTHOR) C.Foullon@exeter.ac.uk, Forsyth, Robert2 (AUTHOR), Barnes, David3 (AUTHOR), Davies, Jackie3 (AUTHOR)
Publikováno v:
Solar Physics. Nov2022, Vol. 297 Issue 11, p1-21. 21p.
Autor:
Gosain, Sanjay, Foullon, Claire
We analyze flare-associated transverse oscillations in a quiescent solar prominence on 8-9 September, 2010. Both the flaring active region and the prominence were located near the West limb, with a favorable configuration and viewing angle. The fulld
Externí odkaz:
http://arxiv.org/abs/1210.6690
We focus on Hinode Solar Optical Telescope (SOT) calcium II H-line observations of a solar quiescent prominence (QP) that exhibits highly variable dynamics suggestive of turbulence. These images capture a sufficient range of scales spatially ($\sim$0
Externí odkaz:
http://arxiv.org/abs/1110.3159
Autor:
Hu, Renyu, Bogdanova, Yulia V., Owen, Christopher J., Foullon, Claire, Fazakerley, Andrew N., Reme, Henri
This paper has been withdrawn by the author since it has been accepted for publishing in J. Geophys. Res. Please contact the American Geophysical Union for the refereed article.
Comment: This paper has been withdrawn
Comment: This paper has been withdrawn
Externí odkaz:
http://arxiv.org/abs/0803.1206
Autor:
Maunder, Megan, Foullon, Claire, Forsyth, Robert, Davies, Emma, Barnes, David, Davies, Jackie
Coronal Mass Ejections (CMEs) and their interplanetary counterparts (ICMEs) are key drivers of space weather throughout the heliosphere. Observational studies are used to understand their evolution and for developing existing models and theory in spa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b517f881875963d24e6e417ab64a314
Autor:
Foullon, Claire (AUTHOR), Malandraki, Olga E. (AUTHOR)
Publikováno v:
Proceedings of the International Astronomical Union. Jul2017, Vol. 13 Issue S335, pb1-b6. 6p.
Autor:
Foullon, Claire (AUTHOR), Malandraki, Olga E. (AUTHOR)
Publikováno v:
Proceedings of the International Astronomical Union. Jul2017, Vol. 13 Issue S335, pf1-f21. 21p.