Scaling laws for the inner structure of the radiation belts. Issue 7 (14th April 2017)
- Record Type:
- Journal Article
- Title:
- Scaling laws for the inner structure of the radiation belts. Issue 7 (14th April 2017)
- Main Title:
- Scaling laws for the inner structure of the radiation belts
- Authors:
- Mourenas, D.
Ma, Q.
Artemyev, A. V.
Li, W. - Abstract:
- Abstract: Accurately modeling the evolution of the electron radiation belts within the plasmasphere represents both an imperative goal for space weather forecasting and a great challenge. Combining previously developed approximate analytical expressions of electron lifetimes with recent statistical models of plasma density, ULF, whistler‐mode, and electromagnetic ion cyclotron waves, we demonstrate that geomagnetic activity and plasma density actually govern the inner structure of the radiation belts through several simple analytical scaling laws when K p < 3. Many of the observed characteristic features of electron fluxes in the energy versus L shell parameter space are straightforwardly explained. In particular, the upper energy limit of significant electron fluxes at L = 1.5 is estimated as ∼1 MeV in agreement with recent satellite observations. This approximate analytical model represents a very simple and powerful tool for exploring and better understanding the complex variations of the inner structure of the radiation belts with geomagnetic activity during relatively quiet times. Key Points: Approximate analytical scaling laws for the inner structure of the radiation belts based on multiple waves and plasma density statistics Scaling laws agree with measured electron lifetimes and electron flux ( E, L ) distributions from the Van Allen Probes Geomagnetic activity and plasmaspheric density are governing the inner structure of the radiation belts through simple scalingAbstract: Accurately modeling the evolution of the electron radiation belts within the plasmasphere represents both an imperative goal for space weather forecasting and a great challenge. Combining previously developed approximate analytical expressions of electron lifetimes with recent statistical models of plasma density, ULF, whistler‐mode, and electromagnetic ion cyclotron waves, we demonstrate that geomagnetic activity and plasma density actually govern the inner structure of the radiation belts through several simple analytical scaling laws when K p < 3. Many of the observed characteristic features of electron fluxes in the energy versus L shell parameter space are straightforwardly explained. In particular, the upper energy limit of significant electron fluxes at L = 1.5 is estimated as ∼1 MeV in agreement with recent satellite observations. This approximate analytical model represents a very simple and powerful tool for exploring and better understanding the complex variations of the inner structure of the radiation belts with geomagnetic activity during relatively quiet times. Key Points: Approximate analytical scaling laws for the inner structure of the radiation belts based on multiple waves and plasma density statistics Scaling laws agree with measured electron lifetimes and electron flux ( E, L ) distributions from the Van Allen Probes Geomagnetic activity and plasmaspheric density are governing the inner structure of the radiation belts through simple scaling laws … (more)
- Is Part Of:
- Geophysical research letters. Volume 44:Issue 7(2017)
- Journal:
- Geophysical research letters
- Issue:
- Volume 44:Issue 7(2017)
- Issue Display:
- Volume 44, Issue 7 (2017)
- Year:
- 2017
- Volume:
- 44
- Issue:
- 7
- Issue Sort Value:
- 2017-0044-0007-0000
- Page Start:
- 3009
- Page End:
- 3018
- Publication Date:
- 2017-04-14
- Subjects:
- radiation belts -- trapped electrons -- hiss -- EMIC -- plasmasphere
Geophysics -- Periodicals
Planets -- Periodicals
Lunar geology -- Periodicals
550 - Journal URLs:
- http://www.agu.org/journals/gl/ ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1002/2017GL072987 ↗
- Languages:
- English
- ISSNs:
- 0094-8276
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4156.900000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 523.xml