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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 left panel displays solar indices (SFI, SN, X-Ray, and 304Å @SEM), geomagnetic indices (A, K Plntry), space weather indices (Ptn Flx, Elc Flx), and other indicators.
- In the middle, there is a "red" image of the current solar corona that represents radiation strength at 304 Ångstrom.
- The right side of the banner displays the calculated HF global conditions. However, the regional conditions vary significanly!
The numerical indices on the left side are explained below:
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 regions
MUF Boulder - Maximum Usable Frequency (MHz) at Boulder, CO, USA, updated every 15 minutes.
The numerical indices on the right side are explained below:
GeoMag - Calculated - Earth`s Geomagnetic based on K-Index. Updated every 3 hours.
Sig Noise - Calculated every ½ hour: S-units (Solar Wind and Geomagnetic Activity)
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