Variation in Plasmaspheric Hiss Wave Power With Plasma Density

[1]  J. Bortnik,et al.  The relationship between the macroscopic state of electrons and the properties of chorus waves observed by the Van Allen Probes , 2016 .

[2]  D. Baker,et al.  Energy‐dependent dynamics of keV to MeV electrons in the inner zone, outer zone, and slot regions , 2016, Journal of geophysical research. Space physics.

[3]  G. Reeves,et al.  Effects of whistler mode hiss waves in March 2013 , 2015 .

[4]  J. Roederer.  On the adiabatic motion of energetic particles in a model magnetosphere , 1967 .

[5]  C. Juang,et al.  Uncertainty of 1‐D Fracture Intensity Measurements , 2017 .

[6]  D. Baker,et al.  Plasmatrough exohiss waves observed by Van Allen Probes: Evidence for leakage from plasmasphere and resonant scattering of radiation belt electrons , 2015 .

[7]  Per-Arne Lindqvist,et al.  Density in the magnetosphere inferred from ISEE 1 spacecraft potential , 1997 .

[8]  J. Borovsky,et al.  Electron loss rates from the outer radiation belt caused by the filling of the outer plasmasphere: the calm before the storm , 2009 .

[9]  Richard B. Horne,et al.  Three‐dimensional electron radiation belt simulations using the BAS Radiation Belt Model with new diffusion models for chorus, plasmaspheric hiss, and lightning‐generated whistlers , 2014 .

[10]  Y. Shprits,et al.  Dependence of plasmaspheric hiss on solar wind parameters and geomagnetic activity and modeling of its global distribution , 2015 .

[11]  G. Cunningham,et al.  Reproducing the observed energy‐dependent structure of Earth's electron radiation belts during storm recovery with an event‐specific diffusion model , 2016 .

[12]  R. Thorne,et al.  Review of radiation belt relativistic electron losses , 2007 .

[13]  C. Mcilwain,et al.  Coordinates for Mapping the Distribution of Magnetically Trapped Particles , 1961 .

[14]  Richard B. Horne,et al.  Calculation of pitch angle and energy diffusion coefficients with the PADIE code , 2005 .

[15]  Jay M. Albert,et al.  Evaluation of quasi-linear diffusion coefficients for whistler mode waves in a plasma with arbitrary density ratio , 2005 .

[16]  R. Horne,et al.  Three‐dimensional ray tracing of VLF waves in a magnetospheric environment containing a plasmaspheric plume , 2009 .

[17]  R. Horne,et al.  Space weather impacts on satellites and forecasting the Earth's electron radiation belts with SPACECAST , 2013 .

[18]  J. Bortnik,et al.  The distribution of plasmaspheric hiss wave power with respect to plasmapause location , 2016 .

[19]  N. Tsyganenko,et al.  Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms , 2005 .

[20]  Y. Nishimura,et al.  Statistical properties of plasmaspheric hiss derived from Van Allen Probes data and their effects on radiation belt electron dynamics , 2015 .

[21]  Craig A. Kletzing,et al.  Fine structure of plasmaspheric hiss , 2014 .

[22]  David G. Sibeck,et al.  Science Objectives and Rationale for the Radiation Belt Storm Probes Mission , 2012, Space Science Reviews.

[23]  N. Meredith,et al.  Plasmaspheric hiss overview and relation to chorus , 2009 .

[24]  J. Bortnik,et al.  Statistical properties of low‐frequency plasmaspheric hiss , 2017 .

[25]  J. Keyser,et al.  The dynamics of the plasmasphere: Recent results , 2013 .

[26]  W. P. Olson,et al.  A quantitative model of the magnetospheric magnetic field , 1974 .

[27]  D. Baker,et al.  The relationship between the plasmapause and outer belt electrons , 2016 .

[28]  R. Horne,et al.  Recent developments in the radiation belt environment model , 2011 .

[29]  M. Spasojević,et al.  New global loss model of energetic and relativistic electrons based on Van Allen Probes measurements , 2016 .

[30]  Richard B. Horne,et al.  Slot region electron loss timescales due to plasmaspheric hiss and lightning‐generated whistlers , 2007 .

[31]  R. J. Strangeway,et al.  The Electric Field and Waves Instruments on the Radiation Belt Storm Probes Mission , 2013 .

[32]  W. Kurth,et al.  Electron densities inferred from plasma wave spectra obtained by the Waves instrument on Van Allen Probes , 2015, Journal of geophysical research. Space physics.

[33]  M. Gkioulidou,et al.  Van Allen Probes investigation of the large‐scale duskward electric field and its role in ring current formation and plasmasphere erosion in the 1 June 2013 storm , 2015 .

[34]  D. Crawford,et al.  The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP , 2013 .

[35]  R. Horne,et al.  Global model of lower band and upper band chorus from multiple satellite observations , 2012 .

[36]  Yuri Shprits,et al.  Three‐dimensional modeling of the radiation belts using the Versatile Electron Radiation Belt (VERB) code , 2009 .

[37]  V. Angelopoulos,et al.  Erosion and refilling of the plasmasphere during a geomagnetic storm modeled by a neural network , 2017 .

[38]  Enrico Camporeale,et al.  Modeling radiation belt electron dynamics during GEM challenge intervals with the DREAM3D diffusion model , 2013 .

[39]  L. Y. Li,et al.  Propagation characteristics of plasmaspheric hiss: Van Allen Probe observations and global empirical models , 2017 .

[40]  Mark B. Moldwin,et al.  A new model of the location of the plasmapause: CRRES results , 2002 .

[41]  L. Kistler,et al.  Simulation of Van Allen Probes plasmapause encounters , 2014 .

[42]  Q. Yan,et al.  Precipitation loss of Van Allen radiation belt electrons by hiss waves outside the plasmasphere , 2018 .

[43]  G. Reeves,et al.  An unusual enhancement of low‐frequency plasmaspheric hiss in the outer plasmasphere associated with substorm‐injected electrons , 2013 .