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Official Journal of the Asia Oceania Geosciences Society (AOGS)

Geoscience Letters Cover Image
Fig. 5 | Geoscience Letters

Fig. 5

From: Effects of the interplanetary magnetic field y component on the dayside aurora

Fig. 5

Latitudinal profiles of auroral energy flux averaged over the 1400–1600 MLT sector for the a Northern and b Southern Hemispheres. In each panel the red trace is for IMF By > 2 nT and the blue trace is for IMF By < − 2 nT. The vertical line segments are one standard deviation of the sample means. c, d Are in the same format as (a, b) but for the prenoon 0900–1100 MLT sector. The insert values R is the red-to-blue energy flux ratio at the flux peak and, in the parenthesis, integrated over the latitude

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