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?
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By Bharat Kunduri
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