Petr

1991 paper
  - First attempt to follow fast pulses
Kasparova et al 2009 setup
  - Initial problem formulation
  * discussion of "constant density" case
  - Karlicky test-particle code, rather than Emslie deterministic propagation
    (ie, get exact particle distribution function)
  * discussion of T/NT distribution function
  - Spitzer conductivity, Peres et al. 1982 thick emission, return current
    (but no He yet)
  * discussion of saturated heat flux (what does the return current do in
   the standard heat-flux scenario?)
  - Return current very important for ionization 
  - Ionization via NLTE
  - 5 level + continuum for H, Fang et al nonthermal rates, time-dependent
    ESE calculation, looks OK
  - MALI technique for RT (Rybicki-Hammer, not Carlsson)
Kasparova et al 2009 results  
  - Ionization lags behind T increase
  - Saha ionization comparison; time-dependent calculation shows long
    recovery time that is quite different; NT rates have striking effect
    at lowest heights (eg 1000 km)
  * Discussion of proton temperature lag (Somov & Syrovatskii)
  - NT effects more important in the wings
  - Contribution functions show clear photospheric contribution in wings
  - Return current (runaway approximation) 
  * Discussion of return-current physics, partial ionization, laboratory
    experience, Langmuir waves etc.
  - Return current losses dominate in upper chromosphere, reduce significance
    of NT
  - Confirm initial decrease of line center H-alpha
  - Ly-alpha shows time scales appearing for no clear reason, some sort
    of echo or resonance due to RT, not hydro?
  * Discussion of TRACE Ly-alpha and UV signatures in this context
Microwave, FIR continua
  - ALMA, SMESE, KOSMA in Tibet
  - H, H- free-free contributions 
  * Discussion of Planck function as source function for continuum
  - Time profiles, NT contributions
  - Attempt to find NT diagnostic tool not so successful
  * Discussion of line-to-continuum ratios for this purpose 
  - Chen, Ding ~2006 on Ca/H signature
Conclusions
  - Comparisons of Halpha, HXR etc on short time scales
    (Wroclaw SETIS observations)
  - Nice cartoon
  * Discussion of Cheng et al. (2006) diagnostic calculations, utility 
    of He lines

Fatima

Introduction
RADYN code 
  - Abbett-Allred modifications
  - F9-F11 calculations
  - Free-streaming limit conduction
Results
  - Constant input until code breaks
  - He plateau develops, non-explosive, hint of TR moving down at end
  * Discussion of upper boundary condition problem and final (cooling) states
  - F10 evolves faster
  - F11 run for about 2 sec
  * Discussion of input function (Karlicky, Fokker-Planck, stochasticity)
  - TRACE predictions
  - TRACE flare data, using correction by 1600A
  -  8-Sep-99 M1.4 example
  - 28-Feb-99 M6.6 example
  - Energetics: 1-2 x 10^22 erg/s total
  * Discussion
  - Ejection 
  - Time history 
  * Discussion of CIV contributions, timing of TRACE data
  - Ly-alpha line profiles from models show two peaks
  * Discussion suggets two velocity components
  - Contribution functions
  * Discussion of blue/red conventions and direction of flows
  - Energetics
  * Discussion of input to Labrosse code
  - Intensities
Conclusions
  - Profiles and energetics agree with observations
  - Want to change heating functions 
  * Discussion of deposition functions 
  - Analysis of contribution functions
  - Addition of CIV etc optically thin