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Space Weather Indices
Measurements of Solar Activity, Aurora, and Other Phenomena.
The strength of present solar X-Ray emisions and geomagnetic field conditions:
| Solar X-Rays | ![]() |
| Geomagnetic Field |
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Present Solar Wind Data |
Northern Auroral Oval |
Souththern Auroral Oval |
Expect good HF propagation when solar wind indications are in the green. When the solar wind magnetic field Bz component goes south and the solar wind speed increases beyond 600 kilometers per second, consider going up on VHF for some auroral DX. HF conditions are likely to be poor on any paths traversing the polar regions. Daytime trans-equatorial paths may be less affected.
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The latest Mauna Loa Solar Observatory Image (Hydrogen Alpha Light). |
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Solar Cycle 24:
The sunspot cycle seems to be off to a slow start,
though the Space Weather Prediction Center ©2005 - 2011 AB9IL, All Rights Reserved. Information: About, Contact Us, Links, Privacy, XML Sitemap, and HTML Sitemap. Again: Content found here may not be copied, re-published, or reproduced without explicit permission. |

