RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 17, ES4003, doi:10.2205/2017ES000606, 2017
Article Map
Time-spatial correspondence between Pi2 wave power and ultra-violet aurora bursts
Figures
- Figure 1. A map of the combined CARISMA-MACCS-MEASURE magnetometer array....
- Figure 2. (a) An image of the auroral UV activation observed by the WIC...
- Figure 3. Left top panel: Time evolution of UV WIC intensity from IMAGE...
- Figure 4. Time evolution of integrated UV auroral intensity (upper panel)...
- Figure 5. Latitudinal distribution on 2000 (day 358) of the particle precipitation...
- Figure 6. (a) An image of the auroral UV activation observed by the WIC...
- Figure 7. Upper panel: Time evolution of UV intensity (integrated over...
- Figure 8. Time evolution of integrated UV auroral intensity (upper panel)...
- Figure 9. (a) Latitudinal distribution on 2001, 02/01 (day 032) of the...
- Figure 10. The latitudinal normalized distribution of UV intensity (during...
- Figure 11. Schematic illustration of the ULF wave energy propagation channels...
- Figure 12. The relative locations of the latitudinal profile of the Pi2...
Tables
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.
Copyright 2017 by the Geophysical Center RAS.
Generated from LaTeX source by ELXpaper, v.1.5 software package.