Local environmental effects on cosmic ray observations at Syowa Station in the Antarctic: PARMA-based snow cover correction for neutrons and machine learning approach for neutrons and muons | Journal of Space Weather and Space Climate

Open Access

Figure 4

Data-model comparison at Syowa Station. (a) Temperatures at 925, 700, 500, 400, 250, 150, 70, 50, and 20 hPa, identical to Figure 3a, (b) neutron count rate in the unit of counts/min, (c) corrected count rate.

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