Ion Kappa Distribution Parameters in the Magnetosphere of the Earth at Geocentric Distances Smaller Than 20 RE During Quiet Geomagnetic Conditions. Issue 10 (29th September 2021)

• Record Type: Journal Article
• Authors: Kirpichev, I. P.; Antonova, E. E.; Stepanova, M.; Eyelade, A. V.; Espinoza, C. M.; Ovchinnikov, I. L.; Vorobjev, V. G.; Yagodkina, O. I.
• Is Part Of: Journal of geophysical research. Volume 126:Issue 10(2021)
• Page Start: n/a
• Page End: n/a
• Publication Date: 2021-09-29
• Subjects: kappa distribution -- magnetosphere -- acceleration and relaxation processes; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2021JA029409
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: The Earth's magnetosphere is mainly a collisionless plasma system with non‐Maxwellian particle distributions, which are often fitted by the kappa function. While the Maxwell distribution function is described by two parameters (density and temperature), the kappa distribution function has three parameters: density, core energy, and the kappa index that characterizes the slope at high energies. In this study, we fitted an ion flux measured by the five Time History of Events and Macroscale Interactions during Substorms satellites in the Earth's magnetosphere during quiet geomagnetic conditions by a single kappa distribution function. The data were constrained to the following regions: from seven Earth Radii (7 R E ) to the Earth's magnetopause at the dayside, and up to 20 R E for other magnetic local time sectors. The two‐dimensional spatial distribution of the fitted parameters and their radial dependencies were analyzed. Regions of high and low κ ‐parameter are selected and their formation is discussed. Key Points: Ion spectra obtained from the Time History of Events and Macroscale Interactions during Substorms satellite mission near the equatorial plane are fitted by a kappa distribution function Distribution of three fitting parameters (density, core energy, value of k characterizing the spectra slope at high energies) are obtained Region of increased k index at geocentric distances 8–10 R E is selected