作者: R.C. Whitten , I.G. Poppoff , J.S. Sims
DOI: 10.1016/0032-0633(71)90203-0
关键词:
摘要: Abstract A model of the positive and negative ion chemistry Martian ionosphere below 80 km is developed. It shown that principal species are expected to be O2+.CO2, H3O+ its hydrates; ions CO3−, CO4− perhaps CO−. The shows Mars above 25 quite insensitive concentrations atomic oxygen ozone, values those rate coefficients have not yet been measured. Below km, sufficient knowledge does exist construct a unique ionospheric model. concluded should very definite D-region permanent low-lying electron layer becomes distinct at night.