RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 17, ES4003, doi:10.2205/2017ES000606, 2017

Figure 7. Upper panel: Time evolution of UV intensity (integrated over the latitudinal and longitudinal range $\Delta \Phi=60.7\mbox{°} -79.1\mbox{°})$ in the LBHL band (solid line) and in the LHBS CARISMA latitudinal profile on 02/01, 2001 (day 032) 0400–0530 UT. CGM latitudes are indicated near station codes. The scale between ticks is shown near left-hand axis. (b) Magnetograms of $X$ component geomagnetic field variations at the high-latitude CARISMA stations (top panel) and at the mid-latitude MEASURE stations (bottom panel) on 02/01, 2001 (day 032) 0420–0450 UT. CGM latitudes are indicated near station codes.

 
Citation: Martines-Bedenko V. A., V. A. Pilipenko, M. J. Engebretson, M. B. Moldwin (2017), Time-spatial correspondence between Pi2 wave power and ultra-violet aurora bursts, Russ. J. Earth Sci., 17, ES4003, doi:10.2205/2017ES000606.
 

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