SDO in Pulkovo Observatory

Details SDO in Pulkovo Observatory SDO in Pulkovo Observatory

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23c1877b&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH23C-1877

Astronomy and Astrophysics

Astrophysics

[7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7536] Solar Physics, Astrophysics, And Astronomy / Solar Activity Cycle, [7549] Solar Physics, Astrophysics, And Astronomy / Ultraviolet Emissions

Scientific paper

We discuss the effective applications of the data obtained with Solar Dynamics Observatory from both instruments: The Helioseismic Magnetic Imager (HMI) and The Atmospheric Imaging Assembly (AIA). The purpose of this presentation is to show the most important problems of solar activity which are the main subjects in the Pulkovo Observatory. There with uniform data sets of magnetic fields and coronal emission in Extreme Ultraviolet bands are needed. Thus, we are planning to create SDO center in the Pulkovo Observatory, which will helps us in collaboration with existed SDO centers and provides more convenient data downloading for solar physics.

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