The Search Coil Magnetometer for THEMIS

By A. Roux, O. Contel, C. Coillot, A. Bouabdellah, B. Porte, D. Alison, S. Ruocco, M. Vassal. 2008

228 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/20ac596c4eeef04eea3df166459f31e977c4d83f

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In Astronomy and Astrophysics

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

In Molecular Biology

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

Citations in the corpus

• Advances in Magnetic Field Sensors (2010, methodology): “Noise of popular EMI induction sensors and a low-noise fluxgate – adapted from a Schlumberger datasheet [54].”
• On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, methodology): “Wave amplitudes of chorus and hiss were obtained from filter bank data (FBK) comprised of the wave magnetic field measured by THEMIS search coil magnetometers (SCM) [Roux et al., 2008].”
• Global distribution of equatorial magnetosonic waves observed by THEMIS (2013, methodology): “…the spin frequency (1/3 Hz) to 4 kHz are measured by the Electric Field Instrument (EFI) [Bonnell et al., 2008] and the Search Coil Magnetometer (SCM) [Roux et al., 2008], respectively, and the Digital Fields Board (DFB) performs data acquisition and signal process thereafter [Cully et al., 2008].”
• First Results from the THEMIS Mission (2008, methodology): “Roux et al., 2008 (this issue).”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, methodology): “The SCM and EFI output waveforms are digitized and processed by the Digital Fields Board (DFB) [Cully et al., 2008].”
• The THEMIS Digital Fields Board (2008, methodology): “The Flux-Gate Magnetometer (FGM) [Auster et al, 2008, this issue] and Search-Coil Magnetometer (SCM) [Roux et al, 2008, this issue] measure the magnetic fields, while the Electric Fields Instrument (EFI) [Bonnell et al, 2008, this issue] measures electric fields.”
• THEMIS observations of long‐lived regions of large‐amplitude whistler waves in the inner magnetosphere (2008, background): “[5] The Digital Fields Board (DFB) (C. M. Cully et al., The THEMIS digital fields board, submitted to Space Science Reviews, 2008) calculates the mean amplitude of the electric and magnetic fields in 6 logarithmically-spaced passbands up to 4 kHz using electric field data from the double-probe Elect”
• Global distribution of whistler‐mode chorus waves observed on the THEMIS spacecraft (2009, methodology): “The Digital Fields Board (DFB) [Cully et al., 2008a] calculates the mean amplitude of the electric and magnetic fields in 6 logarithmically-spaced frequency bands from 0.1 Hz to 4 kHz using electric field data from the double-probe Electric Fields Instrument (EFI) [Bonnell et al., 2008] and magnetic”
• Global model of lower band and upper band chorus from multiple satellite observations (2012, methodology): “Specifically, we thank O. Le Contel and A. Roux for use of SCM data; J. W. Bonnell and F. S. Mozer for use of EFI data; and K. H. Glassmeier, U. Auster, and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through th”