Proton and electron heating by radially propagating fast magnetosonic waves

By R. Horne, G. Wheeler, H. Alleyne. 2000

181 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/bc0025aa3f866c6f3a2b9cc2fcdf0ed7bf35afc5

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. R. Thorne
2. R. Horne
3. Nigel P. Meredith
4. Jacob Bortnik
5. Wen Li
6. S. Glauert
7. Y. Shprits
8. Binbin Ni

In Geophysics

1. R. Thorne
2. Nigel P. Meredith
3. R. Horne
4. Jacob Bortnik
5. S. Glauert
6. Y. Shprits
7. Wen Li
8. Binbin Ni

Citations in the corpus

• Survey of magnetosonic waves and proton ring distributions in the Earth's inner magnetosphere (2008, background): “5 keV protons A number of theoretical studies have shown that magnetosonic waves can be generated 280 by a proton ring distribution in velocity space, or more specifically, a ring corresponding to 281 a positive gradient in the perpendicular velocity distribution of the protons which exceeds 282 the”
• Origins of plasmaspheric hiss (2006, background): “AttenuationintheEarth-ionospherewaveguideofa15.5kHz signal is expected to reduce the wave power by � 3 orders of magnitude over a distance of 1000 km [e.g., Helliwell, 1965, Figure 3.38].”
• Electron acceleration in the Van Allen radiation belts by fast magnetosonic waves (2007, background): “…waves are generated by a proton ring distribution at frequencies close to the harmonics of the proton gyrofrequency [Boardsen et al., 1992, Horne et al., 2000] and can propagate both inside and GEOPHYSICAL RESEARCH LETTERS, VOL. 34, L17107, doi:10.1029/2007GL030267, 2007 1British…”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “The waves are observed both inside and outside the plasmapause and are excited by a cyclotron resonant instability with a ring distribution of injected ring current ions (Horne et al. 2000; Meredith et al. 2008; Chen et al. 2010b).”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “The waves are observed both inside and outside the plasmapause and are excited by a cyclotron resonant instability with a ring distribution of injected ring current ions [Horne et al., 2000].”
• Transit time scattering of energetic electrons due to equatorially confined magnetosonic waves (2010, background): “These observations led early workers to the idea that MS waves derive their energy from a resonant interaction with a highly anisotropic “ring” distribution of energetic protons [e.g.,Gurnett, 1976; Perraut et al., 1982; Boardsen et al., 1992; Horne et al., 2000; Meredith et al., 2008].”
• Global simulation of magnetosonic wave instability in the storm time magnetosphere (2010, background): “When propagation characteristics are considered, the most unstable MS waves occur at a wave normal angle 89.5° [Horne et al., 2000, Figure 9].”
• Global simulation of EMIC wave excitation during the 21 April 2001 storm from coupled RCM‐RAM‐HOTRAY modeling (2010, background): “…ion distribution, which develops during transport and loss, should also be unstable to the excitation of equatorial magnetosonic waves [e.g., Boardsen et al., 1992,Horne et al., 2000] and the quasi‐linear scattering by such waves will also need to be incorporated into the evolving ion distribution.”
• Helium, Oxygen, Proton, and Electron (HOPE) Mass Spectrometer for the Radiation Belt Storm Probes Mission (2013, background): “Generally, five different wave modes can interact strongly with radiation belt electrons (Horne and Thorne 1998) including magnetosonic (Horne et al. 2000) and Z-mode waves (Glauert and Horne 2005).”