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Bruls, J. H. M. J. |
Volume |
Paper Title |
Page Number |
Authors |
26 |
The Chromospheric Temperature Rise in Fluxtubes |
512 |
Bruls, J. H. M. J.; Solanki, S. K. |
64 |
The Non-LTE Formation of Li I Lines from Cool Stars |
270 |
Carlsson, M.; Rutten, R. J.; Bruls, J. H. M. J.; Shchukina, N. G. |
68 |
Magnetic Field Strength and Filling Factor Sensitivity of the MgI 12 MU M Infrared Lines in Solar Plage |
294 |
Bruls, J. H. M. J.; Solanki, S. K. |
109 |
PRD vs. CRD CaII K Stokes profiles from solar plage |
113 |
Bruls, J. H. M. J.; Solanki, S. K.; Uitenbroek, H. |
109 |
Is the optical depth of stellar coronae really negligible? |
289 |
Schrijver, C. J.; Mewe, R.; Kaastra, J. S.; van den Oord, G. H. J.; Bruls, J. H. M. J. |
154 |
A Non-LTE Analysis of Doppler Imaging Lines |
1959 |
Bruls, J. H. M. J.; Solanki, S. K.; Schussler, M. |
158 |
Can Chromospheric Activity mimic a Polar Spot? |
182 |
Bruls, J. H. M. J.; Schüssler, M.; Solanki, S. K. |
223 |
Where is the Intrinsic Size Limit of Fine Structure in the Solar Photosphere? (CD-ROM Directory: contribs/bruls) |
589 |
Bruls, J. H. M. J.; von der Lühe, O. |
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