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Rempel, M. |
Volume |
Paper Title |
Page Number |
Authors |
223 |
Storage of a Strong Magnetic Field Below the Solar Convection Zone (CD-ROM Directory: contribs/rempel) |
738 |
Rempel, M.; Schüssler, M.; Moreno-Insertis, F.; Tóth, G. |
248 |
Intensification of Magnetic Field in a Stellar Convection Zone by Conversion of Potential Energy |
165 |
Rempel, M.; Schüssler, M. |
346 |
Fighting the Taylor-Proudman Constraint - How to Get Differential Rotation Solar-like? |
75 |
Rempel, M. |
346 |
How Sensitive are Rotation Inversions to Subtle Features of the Dynamo? |
99 |
Howe, R.; Rempel, M.; Christensen-Dalsgaard, J.; Schou, J.; Thompson, M.; Komm, R.; Hill, F. |
354 |
The Dynamical Disconnection of Sunspots from their Magnetic Roots |
148 |
Rempel, M.; Schuessler, M. |
358 |
The Uncombed Penumbra |
19 |
Borrero, J.M.; Rempel, M.; Solanki, S.K. |
415 |
Radiative MHD Modeling of Sunspot Fine Structure |
351 |
Rempel, M. |
416 |
Radiative-MHD Simulations of Sunspot Structure |
461 |
Rempel, M. |
416 |
Group Discussion: Solar Activity: The Role of Convection, the Tachocline and the Dynamo and Applications of Data Assimilation |
551 |
Rempel, M.; Dikpati, M. |
456 |
Comparison of Multi-Height Observations with a 3D MHD Sunspot Model |
67 |
Jaeggli, S. A.; Lin, H.; Uitenbroek, H.; Rempel, M. |
463 |
The Sunspot Penumbra in the Photosphere: Results from Forward Synthesized Spectroscopy |
89 |
Tritschler, A.; Uitenbroek, H.; Rempel, M. |
498 |
Solar Differential rotation Maintained by Small- and Large-scale Convection |
154 |
Hotta, H.; Rempel, M.; Yokoyama, T. |
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