What we wish to do:
We looked at the three substorm phases, and the energetic precipitation during that period.
We did this for isolated, multi-onset substorms outside storms. And substorms within storms.
We found the average precipitation spectra for each of these phases, and the average electron ionization profiles.
We evaluated solar-wind driving during these phases, and the corresponding effect of the precipitation.
Guessing what we will find:
Substorm growth phase has some energetic precipitation, that is independent of the strength of the substorms - but rather depends on the storm-recovery phase. CSS depends on the storm recovery phase, as radiation belts are full.
Substorm recovery phase, and multi-onset substorm, have the maximum energetic precipitation.
The proportion of energy within energetic precipitation is highest during recovery phase, and it is ~30% during peak precipitation in the growth phase.
For substorms with storms, energetic precipitation is infact higher than substorms outside storms.
For expansion and recovery phase, the precipitation linearly increases with driving, or AL index.
Conclusion:
Energetic precipitation carries majority of the energy during substorm expansion and recovery phases. And for multi-onset, and ones within storm phases.
Q1 Fig1. Superposed epoch time series with SML and precipitation, with average phase-start and stop times marked. [Similar question in Draft Paper 4: Conductivity contribution of energetic precipitation during substorms]
Q1. Fig 2. Type of substorms flow chart
Q1 Fig3. Average precipitation spectra varying with phase, substorm type, storm flag.
Show, percentage of flux from energetic electrons
Q2 Fig 4. Superposed epoch time-series of average precipitation varying with driving for different substorm types
Q2 Fig 5. SW driving vs. energetic precipitation for different substorm types
A different paper(?)
Q3 Fig 6. Table showing optical signature vs. growth phase precipitation.