Abstract

We evaluate the relative importance of stormtime ring current electrons to protons by calculating the energy content ratio of electrons to protons for typical ring current energies inferred from observations and simulations. We analyze Explorer 45 measurements taken around the minimum Dst(=−171 nT) of the 17 December 1971 storm. We simulate the electron and proton ring current energy content during a hypothetical storm using drift‐loss simulations. From the data analysis, we find that electrons with energies of ∼1–50 keV and protons with energies of ∼10–200 keV contribute the most to the corresponding particle energy content. From both observations and simulations, the ring current electrons contribute only ∼1% as much energy content as ring current protons during quiet times. However, this ratio increases to ∼8–19% during storm main phase. Thus, the ring current electrons can contribute significantly to the ring current energy content during storms.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.