Fig. 8
Comparison of calculated fluxes to PSP observations. The solid line shows the estimated flux of 30 to 40 nm particles relative to PSP, assuming Q/m = 10−6 e∕mp and β = 0.163. To agree with the observed impact rate at the perihelion, the calculated flux had to be multiplied by a factor of 4.5 × 104 cm2. We note thelow flux intensity away from the peak.
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