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Earth, Planets and Space
Fig. 6 | Earth, Planets and Space

Fig. 6

From: Energetic particle flux measurements from the Korean space weather monitor particle detector: a comparative study with the MPS-HI onboard GOES-16

Fig. 6

Energy-based spectral flux distributions with dL* < 0.1 on magnetically quiet days with average Kp index ≤ 2. a Spectral flux distributions for 2020 and 2021 showed good agreement between KSEM PD and MPS-HI, with similar power law distributions, except for Channel 9. The effective energy (Eeff) of GOES-16 MPS-HI electron channels, as determined by Boudouridis et al. (2020), is also included. b Quarterly spectral flux distributions show broader quarterly variation in flux density in KSEM PD, compared with MPS-HI. c Comparisons of the quarterly flux distributions of the two detectors showed narrower variation and higher overall flux in 2021

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