This 22nd volume in the series contains 15 invited reviews and highlight contributions from outstanding speakers presented during the 2009 annual meeting of the Astronomical Society on the subject of "Deciphering the Universe through Spectroscopy", held in Potsdam, Germany.
Topics range from the measurements of magnetic fields on the surface of the sun via detailed measurements of abundances in stellar atmospheres to the kinematics of the universe at its largest scales.
The result is a systematic overview of the latest astronomical and cosmological research.
"synopsis" may belong to another edition of this title.
Regina v. Berlepsch studied Physics at the Friedrich Schiller University in Jena. After finishing her studies, she worked as scientific assistant at the central institute for astrophysics (ZIAP) in Potsdam.
Since 1992, she is leading the scientific documentation center of the Astrophysical Institute in Potsdam (AIP).
This 22nd volume in the series contains 15 invited reviews and highlight contributions presented during the 2009 annual meeting of the Astronomical Society on the topic of "Deciphering the Universe through Spectroscopy".
Spectroscopy is a key method in modern astrophysical research throughout all wavelengths. Applications range from the measurements of magnetic fields on the surface of the Sun over detailed measurements of abundances in stellar atmospheres to the kinematics of the universe on its largest scales. Spectroscopic facilities are key utilities on space and ground based telescopes, and future observational landmarks such as ALMA and the E-ELT primarily focus on spectroscopic methods.
This 22nd volume in the series contains 15 invited reviews and highlight contributions presented during the 2009 annual meeting of the Astronomical Society on the topic of "Deciphering the Universe through Spectroscopy".
Spectroscopy is a key method in modern astrophysical research throughout all wavelengths. Applications range from the measurements of magnetic fields on the surface of the Sun over detailed measurements of abundances in stellar atmospheres to the kinematics of the universe on its largest scales. Spectroscopic facilities are key utilities on space and ground based telescopes, and future observational landmarks such as ALMA and the E-ELT primarily focus on spectroscopic methods.
"About this title" may belong to another edition of this title.
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