Cross Sections

WIP

This section is under construction.

AURORA includes electron-impact cross sections for the three main neutral species in the upper atmosphere: N₂, O₂, and atomic O. For each species, elastic and inelastic (excitation of rotational, vibrational, electronic states and ionization) cross-sections are included.

These data are loaded internally when an AuroraModel is constructed.

Data sources

The cross-section data are primarily based on:

  • Itikawa, Y. (2006). Cross sections for electron collisions with nitrogen molecules. J. Phys. Chem. Ref. Data, 35(1), 31–53.
  • Itikawa, Y. (2009). Cross sections for electron collisions with oxygen molecules. J. Phys. Chem. Ref. Data, 38(1), 1–20.
  • Itikawa, Y. & Ichimura, A. (1990). Cross sections for collisions of electrons and photons with atomic oxygen. J. Phys. Chem. Ref. Data, 19(3), 637–651.

Emission cross sections

In addition to the collision cross sections used by the transport solver, AURORA includes cross sections for specific auroral optical emissions. These are used by make_volume_excitation_file to compute volume excitation rates. The following emission lines are currently implemented:

EmissionSourceWavelengthFunction
N₂⁺ 1NG (0-1)e + N₂4278 Åexcitation_4278
N₂ 1PG (4–1, 5–2)e + N₂6730 Åexcitation_6730_N2
OI 7774 Åe + O7774 Åexcitation_7774_O
OI 7774 Åe + O₂7774 Åexcitation_7774_O2
OI 8446 Åe + O8446 Åexcitation_8446_O
OI 8446 Åe + O₂8446 Åexcitation_8446_O2
O(¹S) green linee + O5577 Åexcitation_O1S
O(¹D) red linee + O6300 Åexcitation_O1D