Enhanced incoherent scatter plasma lines

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Enhanced incoherent scatter plasma lines

Detailed model calculations of auroral secondary and photoelectron distributions for varying conditions have been used to calculate the theoretical enhancement of incoherent scatter plasma lines. These calculations are compared with EISCAT UHF radar measurements of enhanced plasma lines from both the E and F regions, and published EISCAT VHF radar measurements. The agreement between the calcula...

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ژورنال

عنوان ژورنال: Annales Geophysicae

سال: 1996

ISSN: 1432-0576

DOI: 10.1007/s00585-996-1462-z