file: 2010-outline.txt = outline my 2010 Oslo teaching
init: Jun 15 2010 
todo:
    - add NaD Leenaarts

Monday morning
--------------

  open both intro and sumary in two screens, from allpdf  # OK
  open rtsa.pdf in screen left LIT # not used 

  teaching goals 
    fair understanding of EB approximation in photospheric line formation  
      = GRT (hold up)
    fair understanding of effect of scattering on chromospheric lines 
      = RTSA (hold up)

  first find out who of you are thick and who are thin
    who knows EB approximation
    write on board radiation comes out at tau=2/3    poor stellar type
    write on board with = and B and tau=1: I=B(tau=1)
    improve approx, S, tau=mu  I approx Stau=mu)
    when valid?
      need continuous atmosphere thicker than tau=1
    examination  # ended with this
      Na SB display Bruls+Uitenbroek
      EB on blends?
        so many flunked it, I need to start at most basic level
        experts: explain that line center and wing S_c diverge outward
          (Thomson scattering) = problem 7 end of RTSA        


participants
============

Gisela Baumann
Helena Becher
Edgar Carlin
Giorgi Dalakishvili
Ewan Dickinson
Damian Fabbian
Jorge Fuentes
David Graham
Nuno Guerreiro
Jingnan Guo
Kim Hyunnam
Nicolas Labrosse
Anders Lagerfjaard
Ed Lee
Fatima Rubio da Costa
Dan Henrik Sekse
Chunlin Tian
Gregal Vissers
Lotfi Yelles