The THEMIS Digital Fields Board

By Christopher Cully, R. Ergun, K. Stevens, A. Nammari, J. Westfall. 2008

148 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/a2f939cefea2a5b3cbd5b216d8e3253ad67b9496

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In Astronomy and Astrophysics

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

Citations in the corpus

• THEMIS observation of multiple dipolarization fronts and associated wave characteristics in the near‐Earth magnetotail (2009, methodology): “…(SCM), provided magnetic field waveform data with the same resolution as the EFI [Le Contel et al., 2008], (6) The Digital Fields Board (DFB) calculates the mean amplitude of the electric and magnetic fields in 6 logarithmically-spaced frequency bands from 0.1 Hz to 4 kHz [Cully et al., 2008].”
• 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].”
• The Axial Double Probe and Fields Signal Processing for the MMS Mission (2016, methodology): “The THEMIS mission observed fields as high as 500 mV/m (Ergun et al. 2009; Andersson et al. 2009), which provides the basis of the DC range on MMS.”
• The Search Coil Magnetometer for THEMIS (2008, methodology): “A digital command is activated by the DFB (Cully et al. 2008) to connect this signal to the feedback winding of the sensors.”
• The FIELDS Instrument Suite for Solar Probe Plus (2016, methodology): “Further details on the digital filters appear in Cully et al. (2008) and Ergun 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].”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, methodology): “Goldstein and Tsurutani [1984] and Hayakawa et al.”