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Дата изменения: Unknown Дата индексирования: Tue Feb 5 00:35:56 2013 Кодировка: Поисковые слова: солнечная корона |
Duty cycle is typically 5%
Some 
Individual pulses very variable in intensity
Stable profile if several hundred pulses added
Strongly linearly polarised
Monotonic polarisation position angle swing through the pulse implies
the origin is near a magnetic pole
Much more complex polarisation characteristic in msps indicating more
complex field
Very high brightness temperature implies coherent emission
Drifting subpulses
Mode changing