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Modified atomic data for improving the analysis of solar and stellar spectra

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ISSIAtomicData

The goal here is to compute different realizations of the CHIANTI atomic data for use in interpreting observed density sensitive line ratios. Here is a description of the current directories:

  • phase2_20161006 -> Latest versions of emissivities and intensities for CfA meeting

see

  • phase2_20161006/01_chianti_errors -> the latest CHIANTI emissivities
  • phase2_20161006/02_test -> some test data
  • phase2_20161006/03_MHD -> some test data from a MHD simulation [in progress]
  • phase2_20161006/04_observed -> observed EIS intensities
  • phase2_20161006/05_statistics -> R routines for inferring densities

older stuff:

  • atomic_data_v1_hpw -> HPW's calculations with uniform uncertainties
  • atomic_data_v2_gdz -> GDZ's calculations with non-uniform uncertainties (current)
  • chianti_errors_fe_13 -> GDZ's work on Fe XIII
  • chianti_errors_o_7 -> GDZ and CB's work on O VII
  • data/HinodeAnalysisGDZ_v1 -> The analysis of EIS Fe XIII spectra with GDZ atomic data (current)
  • data/HinodeAnalysisHPW_v1 -> Older analysis with HPW atomic data
  • TestR -> A test R script for reading various files

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Modified atomic data for improving the analysis of solar and stellar spectra

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