Real time k-index
Sunspots are cooler areas on the solar surface. These active regions should be carefully watched for possible flare activity. A solar flare releases energy than can affect HF propagation:
- Ionizing radiation that arrives at earth immediatly;
- A supersonic shockwave riding along the solar wind;
- Dense particles behind the shockwave that arrives two to three days after the flare.
X-ray flux levels
A solar flare is an explosion on the Sun. There are 3 categories:
- X-class flares are big; they are major events that can trigger planet-wide radio blackouts and long-lasting radiation storms.
- M-class flares are medium-sized; they can cause brief radio blackouts that affect Earth's polar regions. Minor radiation storms sometimes follow an M-class flare.
- C-class flares are small with few noticeable consequences here on Earth.
Short historical graph of WWV numbers
The solar flux, indicating the level of ionization, affects HF propagation above 10 MHz. The solar flux does not affect 7 MHz and below, since the MUF seldom drops below 10 MHz. The higher the inonization the more reflective our ionosphere is to HF signals, and the higher the MUF. Sunspots are cooler areas on the solar surface. These active regions should be carefully watched for possible flare activity. A index, is derived by averaging the K-index. It ranges from 0-20 for quiet conditions, up to 400 for extreme conditions, representing the overall planetary geomagnetic conditions.
Cycle 23 / Cycle 24 Prediction
Cycle 24 prediction tells us the expected peak and intensity of the sun spot cycle.
CT1BOH - Josť Carlos Cardoso Nunes - email@example.com