Abstract
On the basis of the daily variation of auroras at seven antarctic stations, a diurnal variation of the latitude of maximum auroral activity between approximately 67° and 80° is demonstrated. Northern hemisphere observations suggest that proton precipitation occurs along a similar curve shifted several degrees toward the equator and slightly earlier in time.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
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
