Abstract
view Abstract Citations (2) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Effect of Nongrayness on the Temperature Distribution of the Solar Atmosphere. Münch, Guido Abstract In this paper the temperature distribution in the solar atmosphere is determined by making proper allowance for its departures from grayness. The variation of temperature with optical depth is determined in the second approximation of the method developed by S. Chandrasekhar to solve the problem of radi- ative transfer in a stellar atmosphere in which the continuous absorption coefficient depends on the fre- quency. The difference between this temperature and the gray atmospheric value is found to be sufficiently small to justify the use of the temperature distribution of the gray body as a good first approximation Publication: The Astrophysical Journal Pub Date: March 1948 DOI: 10.1086/145007 Bibcode: 1948ApJ...107..265M full text sources ADS |
Sign-in/Register to access full text options 
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
