Where Do Solar Filaments Form?: Consequences for Theoretical Models

Duncan Hendry Mackay, V Gaizauskas, Anthony Robinson Yeates

Applied Mathematics

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	51-65
Journal	Solar Physics
DOIs	https://doi.org/10.1007/s11207-008-9127-6
Publication status	Published - 2008

Access to Document

10.1007/s11207-008-9127-6

Solar&Magnetospheric Plasma Theory PP/E1: Solar and Magnetospheric Plasma Theory
Neukirch, T. (PI), Hood, A. W. (CoI), Parnell, C. E. (CoI), Priest, E. (CoI), Roberts, B. (CoI) & Wright, A. N. (CoI)
PPARC - Now STFC
1/04/07 → 31/03/12
Project: Standard
PPARC FELOWSHIP-D MACKAY: Dynamic Solar Magnitude Fields
Mackay, D. H. (PI)
PPARC - Now STFC
1/10/04 → 30/09/09
Project: Standard

Cite this

@article{27d94d4598f64f969207aa6757dc20f7,

title = "Where Do Solar Filaments Form?: Consequences for Theoretical Models",

author = "Mackay, {Duncan Hendry} and V Gaizauskas and Yeates, {Anthony Robinson}",

year = "2008",

doi = "10.1007/s11207-008-9127-6",

language = "English",

pages = "51--65",

journal = "Solar Physics",

issn = "0038-0938",

publisher = "Springer",

}