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Fig. 7 | Earth, Planets and Space

Fig. 7

From: Development of an ASIC preamplifier for electromagnetic sensor probes for monitoring space electromagnetic environments

Fig. 7

Measurement (black solid line) and simulation (red dotted line) results for the NEMI for the ASIC preamplifier combined with a 0.01-m\(^{2}\) loop (100 turns). The gray solid line is for the NEMI by a previous preamplifier combined with 0.01-m\(^2\) loop (15 turns) by Yagitani et al. (1994). The dot-dashed line represents the spectral characteristics of the whistler-mode radiation from a Space Shuttle experiment by Gurnett et al. (1986)

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