Survey of magnetosonic waves and proton ring distributions in the Earth's inner magnetosphere

By Nigel P. Meredith, R. Horne, R. R. Anderson. 2008

194 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b1f5d11ac5a86b07bcfc3bec1d3e35b6b1d6f71f

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

In Geophysics

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

In Molecular Biology

1. R. Thorne
2. R. Horne
3. Wen Li
4. Nigel P. Meredith
5. Jacob Bortnik
6. S. Glauert
7. D. N. Baker
8. B. J. Fraser

Citations in the corpus

• Radiation belt dynamics: The importance of wave‐particle interactions (2010, methodology): “CRRES data has been used to confirm the association between MS waves and the presence of ion rings [Meredith et al., 2008].”
• 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].”
• 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).”
• Space Weather Effects in the Earth’s Radiation Belts (2018, unknown): “…waves which are thought to take their energy from enhanced/unstable proton ring current distributions at 10 s of keV energies, as demonstrated by several studies using GOES and CRRES observations among others (Perraut et al. 1982; Meredith et al. 2008; Chen et al. 2016; Balikhin et al. 2015).”
• Relativistic electron loss timescales in the slot region (2009, methodology): “These globally averaged spectral profiles were determined by first averaging the data over the magnetic latitude range 5 Meredith et al., 2008 ], and then over magnetic local time.”
• Global simulation of magnetosonic wave instability in the storm time magnetosphere (2010, background): “tions [Meredith et al., 2008], namely, proton rings on the duskside inside the plamasphere and on the dayside outside the plasmasphere.”
• Global distribution of equatorial magnetosonic waves observed by THEMIS (2013, result): “MS wave amplitudes both inside and outside the plasmapause are stronger at lower magnetic latitudes, consistent with previous studies [e.g. Meredith et al., 2008].”
• Electron losses from the radiation belts caused by EMIC waves (2014, background): “They are thought to be generated by proton ring distributions at energies of about 10 keV [Boardsen et al., 1992] and can propagate both inside and outside the plasmapause [Meredith et al., 2008; Ma et al., 2013].”