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Electron Microburst Size Distribution Derived With AeroCube-6.
M Shumko1, A T Johnson1, J G Sample1
1Department of Physics Montana State University Bozeman MT USA.
Microbursts, sudden electron bursts from radiation belts, are studied for their role in electron loss. This research quantifies microburst sizes, finding most are under 200 km at the magnetic equator.
Area of Science:
- Space Physics
- Plasma Physics
- Atmospheric Science
Background:
- Microbursts are impulsive electron increases from Earth's radiation belts into the atmosphere.
- They are suspected of rapidly depleting radiation belt electrons, but their exact contribution to electron loss is not well understood.
Purpose of the Study:
- To statistically study the size distribution of microbursts.
- To better quantify the role of microbursts in radiation belt electron losses.
Main Methods:
- Utilized data from the AeroCube-6 CubeSat pair for statistical analysis.
- Developed Monte Carlo and analytic models to test microburst size distributions.
- Employed a Markov chain Monte Carlo sampler to estimate optimal model parameters.
Main Results:
- Derived the microburst size distribution in low Earth orbit and at the magnetic equator.
- Observed the majority of microbursts when CubeSat separation was minimal (tens of kilometers).
- Determined that most observed microbursts are less than 200 km in size at the magnetic equator.
Conclusions:
- The study provides a quantified size distribution for microbursts.
- Findings suggest microbursts may play a significant role in radiation belt dynamics.
- Comparison with whistler mode chorus wave distributions offers insights into microburst generation mechanisms.
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