Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/683
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dc.contributor.authorO`Shea, E-
dc.contributor.authorBanerjee, D-
dc.contributor.authorDoyle, J. G-
dc.date.accessioned2006-01-17T06:06:30Z-
dc.date.available2006-01-17T06:06:30Z-
dc.date.issued2005-06-
dc.identifier.citationAstronomy and Astrophysics, Vol. 436, No. 2, pp. L35 - L38en
dc.identifier.urihttp://hdl.handle.net/2248/683-
dc.description.abstractUsing measurements of MgX 609.78 and 624.94 Å lines from the Coronal Diagnostic Spectrometer (CDS) on board SOHO, we seek to examine the variation of line width and line ratio in regions far off-limb at the Northern pole of the Sun. It is found that above ~1150" the ratio of the two coronal MgX resonance lines reduces to values that might be expected for a more radiatively dominant excitation mode. A comparison of the line widths with these ratios indicates that the line widths start to show a decrease in their values at the location where the dominant excitation changes from being collisionally to radiatively dominant, that is, at ~1150". We suggest that the decrease in the line widths above ~1150" is likely to be due to a reduction in the non-thermal component of the line widths caused by a damping of upwardly propagating Alfv´en waves.en
dc.format.extent140088 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Science-
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:200500120-
dc.rights© ESO-
dc.subjectSun: UV Radiationen
dc.subjectSun: coronaen
dc.subjectSun:atmosphereen
dc.titleOn the widths and ratios of MgX 609.79 and 624.94 Å lines in polar off-limb regionsen
dc.typeArticleen
Appears in Collections:IIAP Publications

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