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The Ionospheric Connection Explorer - Prime Mission Review
Thomas J Immel1, Scott L England2, Brian J Harding1
1Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way, Berkeley, 94720-7450 CA USA.
Summary
The NASA Ionospheric Connection Explorer (ICON) mission successfully studied Earth's ionosphere. It revealed how energy from lower and upper atmospheres influences space plasma dynamics, even during solar minimum.
Area of Science:
- Space Physics
- Atmospheric Science
- Plasma Physics
Background:
- The Earth's ionosphere is a dynamic region influenced by solar activity and atmospheric coupling.
- Understanding ionospheric behavior is crucial for space weather prediction and satellite operations.
Purpose of the Study:
- To investigate the mechanisms controlling the ionosphere-thermosphere system using the ICON observatory.
- To analyze the impact of lower and upper atmospheric energy inputs on ionospheric plasma density.
Main Methods:
- The Ionospheric Connection Explorer (ICON) mission collected in-situ and remote sensing measurements.
- Synergistic data collection enabled comprehensive studies of the ionosphere-thermosphere system.
- Observations covered periods of deep solar minimum and increasing solar activity.
Main Results:
- ICON exceeded its mission objectives, providing near-continuous measurements of Earth's densest plasma.
- Remarkable ionospheric effects driven by lower and middle atmospheric energy inputs were elucidated.
- The transmission of energy from space to peak plasma density was observed.
Conclusions:
- ICON's data enhances our understanding of ionospheric variability under varying geomagnetic conditions.
- The mission demonstrated the significant role of atmospheric coupling in ionospheric dynamics.
- ICON's findings contribute to improved space weather models and predictions.
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