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Temporal,seasonal, and solar cycle variations of the topside proton concentration at Arecibo
Institution:1. College of Artificial Intelligence, Nanjing Agricultural University, Nanjing 210031, PR China;2. College of Engineering, Nanjing Agricultural University, Nanjing 210031, PR China;3. School of Physics, Southeast University, Nanjing 211189, PR China
Abstract:An estimate of the topside proton concentration can be obtained by analyzing the incoherent scatter radar autocorrelation function from that region. Our observations at Arecibo, Puerto Rico indicate that the H+ to O+ composition transition height often occurs as low as 450 km during winter nights, near solar minimum. In the summer, the nighttime transition height is only slightly higher, near 600 km. This height is also affected by the level of magnetic activity. Maximum concentrations of H+ occur near 04:00 LT, with a minimum about twelve hours later. The observations of topside H+ were acquired during the past six years as part of the Regular World Day experiments, and from studies of the low latitude hydrogen geocorona. In particular, we will emphasize the results obtained during the solstice and equinox periods of the Thermospheric Mapping Study.
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