Matches in SemOpenAlex for { <https://semopenalex.org/work/W4362469099> ?p ?o ?g. }
- W4362469099 abstract "Collisionless astrophysical plasmas are correlated systems in which particles are often not in thermal equilibrium and can be characterized by power-law distributions. The kappa distribution function, which is a more generalized form of the power-law function, is often used to describe acceleration and production of high-energy particles in different space plasma environments. The spectra of particles in the Earth's plasma sheet constructed using Time History of Events and Mesoscale Interactions during Substorms data show that the kappa index exhibits a strong dawn-dusk asymmetry and a clear dependence on both geocentric distance and magnetic local time. Furthermore, statistics indicate that spectrum hardening, or softening is expected during geomagnetically disturbed periods. To understand how the shape of the particle distribution function evolves and what factors affect the kappa index, we simulate earthward plasma transport using a kinetic drift model. In the simulations, the plasma distribution is initially considered to be a kappa function with . However, with time, both protons and electrons' distribution functions evolve and deviate from their initial shapes. We demonstrate that by implementing transient low-entropy plasma injections, the Rice Convection Model average distribution functions can reasonably agree with observations. We also discuss the relative impact of gradient/curvature drift, particle loss, and bubble injections, based on controlled numerical experiments." @default.
- W4362469099 created "2023-04-05" @default.
- W4362469099 creator A5045365831 @default.
- W4362469099 creator A5054081345 @default.
- W4362469099 creator A5067456688 @default.
- W4362469099 creator A5074706897 @default.
- W4362469099 creator A5077515933 @default.
- W4362469099 creator A5090012516 @default.
- W4362469099 date "2023-04-01" @default.
- W4362469099 modified "2023-10-16" @default.
- W4362469099 title "RCM Modeling of Bubble Injections Into the Inner Magnetosphere: Spectral Properties of Plasma Sheet Particles" @default.
- W4362469099 cites W1495701030 @default.
- W4362469099 cites W1501467981 @default.
- W4362469099 cites W1521098213 @default.
- W4362469099 cites W1573716820 @default.
- W4362469099 cites W1599662942 @default.
- W4362469099 cites W1600243381 @default.
- W4362469099 cites W1613842024 @default.
- W4362469099 cites W1633397315 @default.
- W4362469099 cites W1671244269 @default.
- W4362469099 cites W1710699654 @default.
- W4362469099 cites W1784620720 @default.
- W4362469099 cites W1974468654 @default.
- W4362469099 cites W1974784750 @default.
- W4362469099 cites W1975510234 @default.
- W4362469099 cites W1980947635 @default.
- W4362469099 cites W1992924734 @default.
- W4362469099 cites W1998319939 @default.
- W4362469099 cites W2001486662 @default.
- W4362469099 cites W2004737666 @default.
- W4362469099 cites W2007706441 @default.
- W4362469099 cites W2013158155 @default.
- W4362469099 cites W2016829248 @default.
- W4362469099 cites W2017109395 @default.
- W4362469099 cites W2018454770 @default.
- W4362469099 cites W2019059894 @default.
- W4362469099 cites W2019520795 @default.
- W4362469099 cites W2021637966 @default.
- W4362469099 cites W2023547446 @default.
- W4362469099 cites W2027076235 @default.
- W4362469099 cites W2030775917 @default.
- W4362469099 cites W2031741685 @default.
- W4362469099 cites W2032268555 @default.
- W4362469099 cites W2033652368 @default.
- W4362469099 cites W2034819846 @default.
- W4362469099 cites W2039939942 @default.
- W4362469099 cites W2046507154 @default.
- W4362469099 cites W2050112897 @default.
- W4362469099 cites W2057453691 @default.
- W4362469099 cites W2057794586 @default.
- W4362469099 cites W2060337859 @default.
- W4362469099 cites W2061963596 @default.
- W4362469099 cites W2061969976 @default.
- W4362469099 cites W2063716484 @default.
- W4362469099 cites W2071339788 @default.
- W4362469099 cites W2074062204 @default.
- W4362469099 cites W2077937843 @default.
- W4362469099 cites W2079961019 @default.
- W4362469099 cites W2080109795 @default.
- W4362469099 cites W2081780334 @default.
- W4362469099 cites W2088834317 @default.
- W4362469099 cites W2089456342 @default.
- W4362469099 cites W2093198221 @default.
- W4362469099 cites W2096740924 @default.
- W4362469099 cites W2099041287 @default.
- W4362469099 cites W2101947270 @default.
- W4362469099 cites W2102306644 @default.
- W4362469099 cites W2121307982 @default.
- W4362469099 cites W2133196912 @default.
- W4362469099 cites W2142604100 @default.
- W4362469099 cites W2145655997 @default.
- W4362469099 cites W2146447418 @default.
- W4362469099 cites W2152809278 @default.
- W4362469099 cites W2154820830 @default.
- W4362469099 cites W2158217203 @default.
- W4362469099 cites W2164585288 @default.
- W4362469099 cites W2167986987 @default.
- W4362469099 cites W2171175633 @default.
- W4362469099 cites W2171718596 @default.
- W4362469099 cites W2515839393 @default.
- W4362469099 cites W2563203903 @default.
- W4362469099 cites W2785336214 @default.
- W4362469099 cites W2789581990 @default.
- W4362469099 cites W2809558016 @default.
- W4362469099 cites W2988817865 @default.
- W4362469099 cites W2995302543 @default.
- W4362469099 cites W3009089216 @default.
- W4362469099 cites W3014240186 @default.
- W4362469099 cites W3098946500 @default.
- W4362469099 cites W3104465785 @default.
- W4362469099 cites W3136542076 @default.
- W4362469099 cites W3167940159 @default.
- W4362469099 cites W3201270384 @default.
- W4362469099 cites W4241306035 @default.
- W4362469099 doi "https://doi.org/10.1029/2022ja030673" @default.
- W4362469099 hasPublicationYear "2023" @default.
- W4362469099 type Work @default.
- W4362469099 citedByCount "0" @default.
- W4362469099 crossrefType "journal-article" @default.
- W4362469099 hasAuthorship W4362469099A5045365831 @default.