Images of the Solar Upper Atmosphere From SUMER on SOHO
by Uri Feldman, at al.
Publisher: ESA Publications Division 2003
Number of pages: 209
Investigations of the heating of the corona and the acceleration of the solar wind are two of the prime scientific goals in studying the solar upper atmosphere with the Solar and Heliospheric Observatory (SOHO) of ESA and NASA. The telescope and spectrometer Solar Ultraviolet Measurements of Emitted Radiation (SUMER), one of the twelve scientific instruments aboard SOHO, was designed for spectroscopic studies of the solar chromosphere, transition region, and low corona with emphasis on the dynamics in these regions.
Home page url
Download or read it online for free here:
(multiple PDF files)
by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl - arXiv
The authors focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis on the composition of their ejecta in form of stellar winds during the evolution or of explosive ejecta.
by James Schombert - University of Oregon
This course studies the birth, evolution and death of stars in our galaxy, emphasizing the underlying science behind stellar and galactic evolution, the observational aspect and our knowledge of how the Universe operates on the stellar scale.
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
by George W. Collins, II - W H Freeman & Co
The book on stellar astrophysics for the first year graduates or the advanced undergraduate students. It is assumed that the readers have factual knowledge of stars and astronomy. The text describes the axiomatic theory of stellar structure.