Session Information2005 Joint Assembly |
Solar Physics Division - AAS |
Thursday Morning 1 | |||
| Time | Session | Location | Title |
| 0830 | SP41A | CC Hall B | Corona VI Posters (joint with SH) Presiding: S Bradshaw, Imperial College; D Falconer, Marshall Space Flight Center [Abstracts] |
| 0830 | SP41A-01 | CC Hall B | Heating of the Quiet Solar Corona *V H Hansteen, B W Gudiksen POSTER [details] |
| 0830 | SP41A-02 | CC Hall B | Investigating the Coronal Heating Models at High Resolution *Y Mok, R Lionello, Z Mikic, J Linker POSTER [details] |
| 0830 | SP41A-03 | CC Hall B | Are there two coronal heating mechanisms? *A R Winebarger, H P Warren POSTER [details] |
| 0830 | SP41A-04 | CC Hall B | Coronal Heating Through Reduced MHD Turbulence F Rappazzo, *M Velli, R Dahlburg, G Einaudi POSTER [details] |
| 0830 | SP41A-05 | CC Hall B | Coronal Loop Heating by Nanoflares: The Influence of the Field-aligned Distribution of the Heating on Observables S Patsourakos, *J A Klimchuk POSTER [details] |
| 0830 | SP41A-06 | CC Hall B | Coronal Loop Heating by Nanoflares: Non-thermal Velocities S Patsourakos, *J A Klimchuk POSTER [details] |
| 0830 | SP41A-07 | CC Hall B | Investigation of Solar Coronal Heating Using a Time Dependent MHD Model with Full Conductivity Tensor *F Kazeminezhad, M L Goodman POSTER [details] |
| 0830 | SP41A-08 | CC Hall B | Comparison Between Coronal Loop Solutions and Coronal Scaling Laws *G H Fisher, L L Lundquist, J M McTiernan POSTER [details] |
| 0830 | SP41A-09 | CC Hall B | How does Background Subtraction Affect SXT Loop Temperatures? *J K Roames, J T Schmelz POSTER [details] |
| 0830 | SP41A-10 | CC Hall B | Connectivity of Quiet Sun Magnetic Features *A W Holt, D W Longcope POSTER [details] |
| 0830 | SP41A-11 | CC Hall B | 3D MHD Simulations of Magnetic Flux Emergence in Active Regions *W P Abbett POSTER [details] |