Skip to main content
Earth, Planets and Space
Fig. 8 | Earth, Planets and Space

Fig. 8

From: Evaluation of a method to derive ionospheric conductivities using two auroral emissions (428 and 630 nm) measured with a photometer at Tromsø (69.6°N)

Fig. 8

Comparison of Pedersen conductivities for October 11, 2002; a temporal variations of the height-integrated Pedersen conductivities derived with the EISCAT UHF radar and the photometer observations between 18:00 UT on October 11 and 02:00 UT on October 12, 2002. b Temporal variations of the ratio of the height-integrated Pedersen conductivities from the photometric to radar values

Back to article page