Postdoc research plan

Outline

  • Wrap up SAPS occurrence statistics paper.
  • Statistical model of SAPS velocities.
  • SD - VAP conjugate observations of SAPS.
  • Influence of FACs and equatorward ion and electron precipitation boundary separation on SAPS.

SAPS occurrence statistics paper

  • Expand the existing database of SAPS events (to 2014)
  • Resubmit the paper with the new (expanded) set of SAPS events.

Statistical model of SAPS velocities

  • Apply L-shell fitting to l-o-s velocities for all events in the SAPS database.
  • Obtain statistical variations in SAPS velocities with Dst. (or may be other indicators - IMF?)
  • Compare observations with previous studies
  • Develop a statistical model of SAPS velocities and potential contours.
  • Given a Dst index (or other geomagnetic activity indicator) value, generate estimate of SAPS velocities, potentials - how does it compare with theoretical models?

SD - VAP conjugate observations

  • Develop a database of conjugate SD - VAP SAPS observations.
  • First statistical study showing direct comparison of observations in magnetosphere and ionosphere ?
  • How do SD observations of SAPS electric fields compare with the DC electric fields in VAP?
  • Do the amplitudes and variations in electric fields compare well?
  • What are the influencing factors - Dst, ionospheric conductivity, magnetic mapping ?

Influence of R2 FACs and boundary separation on SAPS

  • From 2015, we can derive ion and electron precipitation boundaries from POES satellite data.
  • AMPERE provides R2 FAC data.
  • R2 FACs should be equatorward of SAPS. Is this the case even for quiet time SAPS? Does this apply only at certain MLTs?
  • Does boundary separation happen at all MLTs and all geomagnetic conditions?
  • How does TEC data compare?
  • What are the factors influencing quiet time SAPS?

pda

By Bharat Kunduri