|
Shchukina, N. G. |
Volume |
Paper Title |
Page Number |
Authors |
26 |
Formation of the MG 112 TTM Lines |
518 |
Carlsson, M.; Rutten, R. J.; Shchukina, N. G. |
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 |
Is LTE a Suitable Approximation for Fe I - based Diagnostics of the Thermal Structure of Sunspots? |
207 |
Shchukina, N. G.; Trujillo Bueno, J. |
118 |
The Instrumentation of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine |
372 |
Kostik, R. I.; Shchukina, N. G. |
223 |
Simulation of Temporal Variations of the Solar Line Fe I 532. 4185 nm by the 5-min Oscillations (CD-ROM Directory: contribs/khomenko) |
680 |
Khomenko, E. V.; Shchukina, N. G. |
223 |
Fe I Lines in the Spectra of Solar-like Stars: NLTE Effects, Temperature Diagnostics and the Iron Abundance (CD-ROM Directory: contribs/shchukin) |
868 |
Shchukina, N. G.; Trujillo Bueno, J. |
|
|