Multipoint observations of magnetospheric compression‐related EMIC Pc1 waves by THEMIS and CARISMA

By M. Usanova, Ian R. Mann, I. J. Rae, Z. Kale, V. Angelopoulos, John W. Bonnell, K. Glassmeier, H. Auster, H. Singer. 2008

156 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e6118adeb2bb856af6c0d3e36f21b904cae48e71

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In Astronomy and Astrophysics

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

In Molecular Biology

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

Citations in the corpus

• Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “…include the overlap between the ring current and the plasmasphere [Pickett et al., 2010], dayside drainage plumes [Morley et al., 2009], and the outer dayside magnetosphere in association with solar wind pressure fluctuations [Arnoldy et al, 2005; Usanova et al., 2008; McCollough et al., 2009].”
• On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, background): “Since EMIC waves are often generated during magnetospheric compressions [e.g., Usanova et al., 2008; 2012, and references therein], we also considered the possibility of EMIC-related loss of MeV electrons to the atmosphere.”
• Circulation of Heavy Ions and Their Dynamical Effects in the Magnetosphere: Recent Observations and Models (2014, background): “EMIC waves are excited by a ring current temperature anisotropy with characteristic amplitudes of up to 10 nT during geomagnetically active conditions (e.g., Cornwall 1965; Søraas et al. 1980; Usanova et al. 2008, 2012; McCollough et al. 2010).”
• Global characteristics of electromagnetic ion cyclotron waves: Occurrence rate and its storm dependence (2013, background): “For the EMIC wave event on 29 June 2007 [Mann et al., 2008;Usanova et al., 2008],McCollough et al. [2010] demonstrated that enhanced ion anisotropies can be created in offequatorial, minimum-B pockets because of drift shell splitting as well as drift orbit bifurcation [McCollough et al., 2012].”
• Global morphology and spectral properties of EMIC waves derived from CRRES observations (2014, background): “…which occurs during geomagnetic storms and substorms [Cornwall et al., 1970; Jordanova et al., 2001] and in the outer dayside magnetosphere, where they have been found to be associated with solar wind pressure fluctuations [Anderson and Hamilton, 1993; Arnoldy et al., 2005; Usanova et al., 2008].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “EMIC waves are intense electromagnetic emissions, which typically occur in distinct frequency bands below ion cyclotron frequencies (Engebretson et al., 2002; Erlandson & Ukhorskiy, 2001; Fraser et al., 2010; Min et al., 2012; Usanova et al., 2008), and sometimes exhibit discrete, coherent structure”
• Resonant scattering of outer zone relativistic electrons by multiband EMIC waves and resultant electron loss time scales (2015, background): “The compression of the magnetopause is suggested as another possible source of EMIC waves [e.g., Anderson and Hamilton, 1993; McCollough et al., 2012; Usanova et al., 2008].”