S/WAVES: The Radio and Plasma Wave Investigation on the STEREO Mission
By J. Bougeret, K. Goetz, M. Kaiser, S. Bale, P. Kellogg, M. Maksimović, N. Monge, S. Monson, P. Astier, S. Davy and 33 more. 2008
370 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Oceanography
View Paper: https://www.semanticscholar.org/paper/cf6d2df0d5065762b6f5ee92f62845998752633f
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Citations in the corpus
- The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories (2008, methodology): “(2007), the SWAVES instrument by Bougeret et al. (2007), and the IMPACT instrument suite by Luhmann et al.”
- SunPy—Python for solar physics (2015, background): “Currently, the Spectrogram class supports radio spectrograms from the e-Callisto ( http://www.e-callisto.org/) solar radio spectrometer network (Benz et al., 2009) and STEREO/SWAVES spectrograms (Bougeret et al., 2008).”
- The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event (2012, methodology): “Signatures of radio bursts are detected with the WAVES instrument aboard WIND (Bougeret et al., 1995) and the STEREO/WAVES instruments (Bougeret et al., 2008).”
- A review of solar type III radio bursts (2014, methodology): “More recent observations of clumpy Langmuir waves show similar properties (e.g. Kellogg et al., 2009) using the time domain sampler in the WAVES instrument onboard the STEREO spacecraft (Bougeret et al., 2008).”
- Dust Detection by the Wave Instrument on STEREO: Nanoparticles Picked up by the Solar Wind? (2009, methodology): “The S/WAVES instrument (Bougeret et al., 2008) onboard the STEREO spacecraft was designed to study solar radio emissions and solar wind plasma waves.”
- Solar flares, coronal mass ejections and solar energetic particle event characteristics (2016, methodology): “From 2006, onwards, we further used composite radio spectra from STEREO/SWAVES (Bougeret et al. 2008), to achieve better identification of events behind the limb.”
- The FIELDS Instrument Suite for Solar Probe Plus (2016, methodology): “FIELDS will make electric field measurements both as a current-biased resistively-coupled doubleprobe instrument (Harvey et al. 1995; Bonnell et al. 2009; Wygant et al. 2013) and as a capacitively-coupled radio and plasma wave instrument (Bougeret et al. 1995, 2008).”