2.3.0 spase://JAXA/NumericalData/Akebono/LEP/PT8S Akebono LEP ion and electron count rates 2021-03-02T17:39:48Z These data consist of ion and electron count rates taken in 18 pitch angle directions and in 29 energy channels between 10eV and 16keV (electrons) or 13ev/Q and 20keV/Q (ions). A full distribution is available each 8 seconds. Through the DARTS/LEP interface, one specifies a particular 10-deg-wide pitch angle bin and retrieves tables of ion and electron count rates with columns for the energy channels and one row for each 8-sec interval. There are companiog plots with spectrograms showing count rates vs. energy and time, one such plot for each of several ~30deg-wine pitch angle bins In any publications, the use of the Akebono data should be acknowledged, for example, as "Akebono LEP data were provided by T. Mukai through DARTS at Institute of Space and Astronautical Science, JAXA in Japan." spase://SMWG/Person/Toshifumi.Mukai PrincipalInvestigator DARTS_LEP readme https://www.stp.isas.jaxa.jp/akebono/readme/readme.lep.txt spase://VSPO/NumericalData/Akebono/LEP/PT8s spase://VSPO/NumericalData/Akebono/LEP/PT8S spase://SMWG/Repository/DARTS Online Open DARTS_JAXA https://www.darts.isas.ac.jp/stp/akebono/LEP.html Text In any publications, the use of the Akebono data should be acknowledged, for example, as "Akebono LEP data were provided by T. Mukai through DARTS at Institute of Space and Astronautical Science, JAXA in Japan." Uncalibrated spase://SMWG/Instrument/Akebono/LEP ThermalPlasma 1989-04-15T00:00:00 1997-12-26T00:00:00 PT8S Earth.NearSurface.AuroralRegion LEP count rate data may still contain background noise depending on pitch angles. The data less than 1000 cps may be unreliable. Those less than 300 cps may be very unreliable.