|
Size: 841
Comment:
|
Size: 1005
Comment: converted to 1.6 markup
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 12: | Line 12: |
| === list of papers having been discussed === [for 05/13/2011 ] |
=== list of papers discussed already === |
| Line 15: | Line 14: |
| [05/20/2011] * Magneto-thermal convection in solar prominences : T. Berger et al., http://www.nature.com/nature/journal/v472/n7342/full/nature09925.html (K.Hayashi) [05/13/2011 ] |
|
| Line 18: | Line 21: |
| [:../: go back to the Group Meeting page] | [[../| go back to the Group Meeting page]] |
Stanford Solar Group Meetings
since 05/13/2011
list of papers discussed already
[05/20/2011]
Magneto-thermal convection in solar prominences : T. Berger et al., http://www.nature.com/nature/journal/v472/n7342/full/nature09925.html (K.Hayashi)
[05/13/2011 ]
Solar models with accretion. I. Application to the solar abundance problem Authors: Aldo M. Serenelli, Wick C. Haxton, Carlos Pena-Garay,http://arxiv.org/abs/1104.1639 (A.Kosovichev)
Evidence for solar frequency dependence on sunspot type Authors: Charles S. Baldner, Richard S. Bogart, and Sarbani Basu, http://adsabs.harvard.edu/abs/2011ApJ...733L...5B (K. Nagashima)