... Future seminars . ... G.V. Levina (Institute of Continuous Media Mechanics) . ... Abstract . ... The INTEGRAL mission and its first results" . ... Reconnection - new basic results and solar simulations " . October, 30 . ... D.L. Vainchtein (IKI RAN; Dept. of Mechanical and Environmental Engineering, University of California Santa Barbara, USA) . ... New results on Solar Structure and Dynamics and Solar Space Observatories " . ... E.B. Gliner (Theoretial Research Institute, San Francisco) . ...

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... We proposed that information retrieved from the local surface photometric behavior of the Moon could be used for guiding the remote sensing analyses of specific geological targets. ... The value of the difference of intensities mentioned above may be used as a photometric parameter I of the local surface roughness. ... 7] Apollo 11 Prelim. ... Figure 5 represents the diagram of relationship between photometric roughness parameter and local thorium content in different lunar regions. ...

... Arefiev, Vadim - Space Research Institute (IKI), Russia . ... Becker, Werner - Max Planck Institute for Extraterrestrial Physics, Germany . ... Bergemann, Maria - Max-Planck Institute for Astrophysics, Germany . ... Tuebingen, Germany . ... Lyskova, Natalya - Max Planck Institute for Astrophysics, Germany; Space Research Institut (IKI), Russia . ... First eROSITA International Conference: Mapping the Structure of the Energetic Universe 17-20 Oct 2011, Garmisch-Partenkirchen (Germany) . ...

... National Institute of Astrophysics) in collaboration with the National . Institute of Nuclear Physics, and will consist of Invited Talks and Joint . ... Astrophysics . ... F. Pacini (chair), M. Baldo Ceolin, R. Barbieri, C. Cesarsky, A. Gimenez, . ... M. Salvati (chair), R. Bandiera, L. Falai, R. Maiolino, F. Mannucci, . ... email: texas_florence@arcetri.astro.it . fax: +39 055 220039 . ... Last updated September 12, 2002 . ...

Magnetic stars, 2004,225-229 Averaged magnetic phase curves. ... ANALYSIS OF THE CATALOG 227 4 3 N stars 2 1 -4000 -3000 -2000 -1000 0 1000 2000 B0 (G) Figure 3: Number distribution of stars vs. coeffcient B0 for those stars which exhibit a magnetic phase curve with a double wave. of a magnetic star can occur if the angle between the magnetic and rotational axes is small or even zero. ... The catalog lists phase curves for 139 stars, 134 of them are magnetic Ap stars. ...