@misc{Ogilvie_Merka_Vinas_Fitzenreiter_2021, title={Wind Solar Wind Experiment (SWE) Electron Pitch-Angle Distributions (12-15s rate) (New Model)}, url={https://hpde.io/NASA/NumericalData/Wind/SWE/H3/PT12S}, DOI={10.48322/XDPR-7352}, abstractNote={Wind SWE electron pitch angle product providing electron fluxes at 30 directional bins relative to the instantaneous magnetic field direction at 13 different energy levels from a later mode (post-VEIS-era) of the electron instrument. The electron pitch-angle distributions included in this data set are derived from sorting, by pitch (with respect to B) and energy, the solar wind electron distributions measured by the Wind/SWE electron instrument . Pitch-angle distributions, organized by energy, are computed from 9s measurements which are usually separated by one or more 3s spin-periods. These quantities are reliable and citable with caution, meaning that the PI advises that the user should discuss their interpretations with a member of the SWE science team before publishing. }, publisher={NASA Space Physics Data Facility}, author={Ogilvie, Keith W. and Merka, Jan and Vinas, Adolfo F. and Fitzenreiter, Richard J.}, year={2021} }