The equatorial latitude of auroral activity during 1972 1977
Abstract
The equatorial latitude of auroral activity has been derived from both electron and optical observations with the DMSP satellites. Virtually all of the observations that were obtained during the 5-year interval June 1972-September 1977 have been used to construct a nearly continuous plot of invariant geomagnetic latitude versus time.
- Publication:
-
Solar Physics
- Pub Date:
- August 1980
- DOI:
- 10.1007/BF00146693
- Bibcode:
- 1980SoPh...67..189S
- Keywords:
-
- Auroras;
- Geomagnetic Latitude;
- Magnetic Equator;
- Meteorological Satellites;
- Satellite Observation;
- Coronal Holes;
- Diurnal Variations;
- Earth Axis;
- Earth Rotation;
- Interplanetary Magnetic Fields;
- Magnetic Poles;
- Solar Flares;
- Geophysics;
- Flare;
- Solar Flare;
- Coronal Hole;
- Interplanetary Magnetic Field;
- Geomagnetic Latitude;
- Aurorae:Activity