Solar conditions like sunspot activity, solar flares, and coronal mass ejections influence Earth's ionosphere, altering its density and structure. These changes affect skywave propagation by enhancing or disrupting radio signal reflection, especially in HF bands used for long-distance communication. Solar activity, governed by the solar cycle, impacts radio skywave propagation on Earth. When solar activity is high (such as during solar flares or geomagnetic storms), an increase in sunspots enhances the ionosphere's ability to refract radio waves. Conversely, during periods of low solar activity, a decrease in sunspots diminishes this refractive capacity, negatively impacting global communication. The careful selection of suitable ham bands is therefore crucial to the success of ham radio operations. Amateur radio operators use solar indices to predict radio wave behavior and adjust communication strategies. See for example the following banner courtesy of Paul L Herrman, N0NBH: This banner is separated into three sections:
The numerical indices on the left side are explained below: SFI - Solar Flux, 2800MHz (10.7cm) ↗ (SFU units) correlates with F2-region ionization; higher value better HF conditions.
SN - Daily Sunspot Number is a measure of the solar activity; like SFI it correlates with enhanced F2-region i.e. better HF conditions
K-Index↗: Geomagnetic Disturbance; good conditions K < 3 | A -Index↗: 24 hours Average; good conditions A < 10
304 Å: Total Solar Radiation at SEM (Solar EUV Monitor) wavelenth: 304 Ångstroms (30.4nm) that affects F-region ionization
Ptn - Proton Flux Density | Elc - Electron Flux Density in the Solar Wind;
both impact E-region
Aurora indicates the strength of the ionization of the F-region in the polar regionsMUF Boulder - Maximum Usable Frequency (MHz) at Boulder, CO, USA, updated every 15 minutes.
The numerical indices on the right side are explained below: The project "Understanding HF Propagation" focuses on near-real-time indicators and explains what they mean.
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