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Fig. 19 | Earth, Planets and Space

Fig. 19

From: Exploration of energization and radiation in geospace (ERG): challenges, development, and operation of satellite systems

Fig. 19

Summary of all mission data recorded on December 20, 2017. The top four panels show the temporal variation in the plasma wave power spectra: a the electric field power spectra at 10 kHz–10 MHz as recorded by the PWE high-frequency analyzer (HFA), b the electric field and c the magnetic field power spectra at 10 Hz–20 kHz recorded by the PWE onboard frequency analyzer, and d the electric field power spectra at DC-200 Hz recorded by the electric field detector. The next six panels show the temporal variation in the particle energy spectra of e 400 keV–20 MeV electrons as recorded by the XEP, f 70 keV–1 MeV particles as recorded in the high-energy particle experiments, g 10–80 keV electrons as recorded by the MEP-e, h 19 eV–19 keV electrons as recorded by the LEP-e, i 10–180 keV/q ions as recorded by the MEP-i, and j 10 eV/q–25 keV/q ions as recorded by the LEP-i. The bottom panel k shows the DC magnetic field recorded in the MGF experiments. The white blanks in panels aj represent no or insufficient data or observations or observations made in a mode other than the observation mode. For example, during the long blanks shown in the ion measurements in (i) and (j), the ion analyzers were in TOF mode to conduct high-resolution ion composition measurements

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