Comparison of the characteristic energy of precipitating electrons derived from ground-based and DMSP satellite data
International audience Energy maps are important for ionosphere-magnetosphere coupling studies, because quantitative determination of field-aligned currents requires knowledge of the conductances and their spatial gradients. By combining imaging riometer absorption and all-sky auroral optical data i...
| Main Authors: | , , |
|---|---|
| Other Authors: | |
| Format: | Article in Journal/Newspaper |
| Language: | English |
| Published: |
HAL CCSD
2005
|
| Subjects: | |
| Online Access: | https://hal.science/hal-00317498 https://hal.science/hal-00317498/document https://hal.science/hal-00317498/file/angeo-23-135-2005.pdf |
| Summary: | International audience Energy maps are important for ionosphere-magnetosphere coupling studies, because quantitative determination of field-aligned currents requires knowledge of the conductances and their spatial gradients. By combining imaging riometer absorption and all-sky auroral optical data it is possible to produce high temporal and spatial resolution maps of the Maxwellian characteristic energy of precipitating electrons within a 240240 common field of view. These data have been calibrated by inverting EISCAT electron density profiles into equivalent energy spectra. In this paper energy maps produced by ground-based instruments (optical and riometer) are compared with DMSP satellite data during geomagnetic conjunctions. For the period 1995-2002, twelve satellite passes over the ground-based instruments' field of view for the cloud-free conditions have been considered. Four of the satellite conjunctions occurred during moderate geomagnetic, steady-state conditions and without any ion precipitation. In these cases with Maxwellian satellite spectra, there is 71% agreement between the characteristic energies derived from the satellite and the ground-based energy map method. |
|---|