The MMS magnetic field power spectral density (BPSD) is computed onboard by the Digital Signal Processor (DSP). The fast Fourier transform (FFT) calculation is performed on a digitized version of anal
A software used to study Earth's dayside magnetosphere is published.To reproduce the result presented in the article, you need to:- Assemble and link the source files using `make`. Refer to `src/READM
Plasmaspheric hiss is a broadband incoherent whistler mode emission with frequencies ranging from ~20 Hz to ~2 kHz, which is observed predominantly inside the plasmasphere. Hiss waves can efficiently
Averaged Wind SWE electron pitch angle data (12-15 seconds rate) from a later mode (post-VEIS-era) of the electron instrument. The electron pitch-angle distribution averages included in this data set
