Characterization and Modeling of Solar Flare Effects in the Ionosphere Observed by HF Instruments
The ionosphere is the conducting part of the upper atmosphere that plays a significant role in trans-ionospheric high frequency (HF, 3-30 MHz) radiowave propagation. Solar activities, such as solar flares, radiation storms, coronal mass ejections (CMEs), alter the state of the ionosphere, a phenomen...
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Virginia Tech
2021
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Online Access: | http://hdl.handle.net/10919/103706 |