Observation of chorus waves by the Van Allen Probes: Dependence on solar wind parameters and scale size

TitleObservation of chorus waves by the Van Allen Probes: Dependence on solar wind parameters and scale size
Publication TypeJournal Article
Year of Publication2016
AuthorsAryan, H, Sibeck, D, Balikhin, M, Agapitov, O, Kletzing, C
JournalJournal of Geophysical Research: Space Physics
Volume121
Issue8
Pagination7608 - 7621
Date Published08/2016
Keywordsdistribution of chorus wave intensities in the inner magnetosphere; inner magnetosphere; Radiation belts; scale size of chorus wave packets; Van Allen Probes; wave-particle interaction
AbstractHighly energetic electrons in the Earth's Van Allen radiation belts can cause serious damage to spacecraft electronic systems and affect the atmospheric composition if they precipitate into the upper atmosphere. Whistler mode chorus waves have attracted significant attention in recent decades for their crucial role in the acceleration and loss of energetic electrons that ultimately change the dynamics of the radiation belts. The distribution of these waves in the inner magnetosphere is commonly presented as a function of geomagnetic activity. However, geomagnetic indices are nonspecific parameters that are compiled from imperfectly covered ground based measurements. The present study uses wave data from the two Van Allen Probes to present the distribution of lower band chorus waves not only as functions of single geomagnetic index and solar wind parameters but also as functions of combined parameters. Also the current study takes advantage of the unique equatorial orbit of the Van Allen Probes to estimate the average scale size of chorus wave packets, during close separations between the two spacecraft, as a function of radial distance, magnetic latitude, and geomagnetic activity, respectively. Results show that the average scale size of chorus wave packets is approximately 1300–2300 km. The results also show that the inclusion of combined parameters can provide better representation of the chorus wave distributions in the inner magnetosphere and therefore can further improve our knowledge of the acceleration and loss of radiation belt electrons.
URLhttp://doi.wiley.com/10.1002/2016JA022775
DOI10.1002/jgra.v121.810.1002/2016JA022775
Short TitleJ. Geophys. Res. Space Physics


Page Last Modified: September 20, 2016