THEMIS observations of long‐lived regions of large‐amplitude whistler waves in the inner magnetosphere

By Christopher Cully, John W. Bonnell, R. Ergun. 2008

146 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/e1bfe1594b8b1692c0048819bb5c4c5549a36a71

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. Jacob Bortnik
4. Binbin Ni
5. Nigel P. Meredith
6. R. Horne
7. Y. Shprits
8. V. Angelopoulos

In Geophysics

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

Citations in the corpus

• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “large‐amplitude chorus (e.g., Cattell et al., 2008; Cully et al., 2008; Kellogg et al., 2011; Tyler et al., 2019; Wilson et al., 2011), test particle simulations have demonstrated its general validity for small amplitude and broadband waves (Tao et al.”
• Global model of lower band and upper band chorus from multiple satellite observations (2012, methodology): “The high resolution (fff) data used here consists of measurements of one component of the magnetic wave spectral density in the spacecraft spin plane, with a frequency resolution with 32 or 64 frequency bands logarithmically spaced over 4–4000 Hz [Cully et al., 2008a].”
• Nonlinear interaction of energetic electrons with large amplitude chorus (2008, background): “[6] Here, we study the wave-particle interactions at L = 5 since this is the region where the largest amplitude chorus waves are present [Cully et al., 2008], maximum inferred internal acceleration occurs [Green and Kivelson, 2004],”
• Fine structure of large‐amplitude chorus wave packets (2014, background): “…Substorms, and Wind) have subsequently revealed that whistler mode waves with electric fields up to a few hundred mV/m can exist in the inner magnetosphere [Cattell et al., 2008; Cully et al., 2008; Kellogg et al., 2011] although their properties sometimes show distinct differences from chorus.”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, background): “However, in a recent statistical study using the THEMIS filter bank wave data, Li et al. [2009a] found that nightside chorus waves tend to maximize at L < 7 and become weak or disappear at L > ∼8.”
• The Electric Field Instrument (EFI) for THEMIS (2008, methodology): “Note that while the short axial booms do lead to significant issues with the DC field measurement, the AC field mea- surement (above a few hundred Hz) does not suffer from these failings, and has been used to make clean, three-dimensional E-field estimates successfully (e.g. Cully et al. 2008a).”
• Global distribution of whistler‐mode chorus waves observed on the THEMIS spacecraft (2009, methodology): “The resulting wave amplitudes (filter bank data) are included in the survey mode telemetry, covering most orbits with a measurement cadence of four seconds [Cully et al., 2008a].”
• Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, background): “The obtained spatial distributions are consistent with the earlier plasmaspheric hiss observations aboard DE-1 [André et al., 2002; Green et al., 2005] and aboard CRRES [Meredith et al., 2004], and lower band chorus statistics from CRRES [Meredith et al., 2001], THEMIS [Cully et al., 2008; Li et al.”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, unknown): “%) of occurrence [Cully et al., 2008].”