Abstract
AbstractIt is argued that detailed consideration of the 24‐hour waveform of ozone in the upper stratosphere provides a means of testing current photochemical kinetic mechanisms, with measurements requiring good relative rather than good absolute accuracy. The implications of the pronounced changes with height of the waveform for remote sounding and monitoring are pointed out. Diurnal, semidiurnal and higher harmonics of ozone and temperature waveforms are obtained by Fourier analysis.
Full Text
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call