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Rutten, R. J. |
Volume |
Paper Title |
Page Number |
Authors |
26 |
Dynamics of the Quiet Solar Atmosphere: K2v Cell Grains Versus Magnetic Elements |
161 |
Brandt, P. N.; Rutten, R. J.; Shine, R. A.; Trujillobueno, J. |
26 |
Formation of the MG 112 TTM Lines |
518 |
Carlsson, M.; Rutten, R. J.; Shchukina, N. G. |
46 |
SIMURIS: High-Resolution Solar Physics |
184 |
Rutten, R. J.; Dame, L. |
46 |
Oscillations of the Magnetic Network |
530 |
Lites, B. W.; Rutten, R. J.; Kalkofen, W. |
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. |
78 |
The Determination of the Solar Iron Abundance from Fe I Lines |
399 |
Kostik, R. I.; Shchukina, N. G.; Rutten, R. J. |
118 |
First Results from SOHO on Waves Near the Solar Transition Region |
284 |
Steffens, S.; Deubner, F.-L.; Fleck, B.; Wilhelm, K.; Schuhle, U.; Curdt, W.; Harrison, R.; Gurman, J.; Thompson, B. J.; Brekke, P.; Delaboudiniere, J.-P.; Lemaire, P.; Hessel, B.; Rutten, R. J. |
118 |
Chromospheric Dynamics and the FIP Flip |
298 |
Rutten, R. J. |
118 |
Dutch Open Telescope: Status and Prospects |
335 |
Rutten, R. J.; Hammerschlag, R. H.; Bettonvil, F. C. M. |
158 |
The Dutch Open Telescope |
57 |
Rutten, R. J.; Hammerschlag, R. H.; Bettonvil, F. C. M. |
158 |
Dynamics of the Quiet Solar Chromosphere |
249 |
Rutten, R. J.; Lites, B. W.; Berger, T. E.; Shine, R. A. |
158 |
Radiative Transfer for Grabs |
306 |
Rutten, R. J. |
183 |
Internetwork Grains with TRACE |
383 |
Rutten, R. J.; de Pontieu, B.; Lites, B. |
184 |
(Inter-),Network Structure and DynamicS |
181 |
Rutten, R. J. |
223 |
Solar Atmospheric Dynamics (CD-ROM Directory: contribs/rutten) |
117 |
Rutten, R. J. |
236 |
Proxy Magnetometry with the Dutch Open Telescope |
25 |
Rutten, R. J.; Hammerschlag, R. H.; Sütterlin, P.; Bettonvil, F. C. M. |
236 |
A Multi-Channel Speckle Imaging System for the DOT |
431 |
Sütterlin, P.; Hammerschlag, R. H.; Bettonvil, F. C. M.; Rutten, R. J.; Skomorovsky, V. I.; Domyshev, G. N. |
236 |
Proxy Magnetometry of the Photosphere: Why are G-Band Bright Points so Bright? |
445 |
Rutten, R. J.; Kiselman, D.; Rouppe van der Voort, L.; Plez, B. |
288 |
Utrecht Radiative Transfer Courses |
99 |
Rutten, R. J. |
288 |
NLTE in a Hot Hydrogen Star: Auer & Mihalas Revisited |
130 |
Wiersma, J.; Rutten, R. J.; Lanz, T. |
470 |
Twists to Solar Spicules |
49 |
Rutten, R. J. |
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