Solar & Propagation
A simple, self-contained guide to interpreting common HF, VHF and UHF propagation conditions. No live feed or outside service is required.
Solar Flux Index & Kp
Lower HF bands may still perform well, especially at night.
Improved opportunities on 20–10 meters depending on path and time.
Higher HF bands can become very productive when geomagnetic conditions cooperate.
Generally favorable for stable propagation, including many longer paths.
Some paths may weaken or become less predictable.
HF propagation may be disturbed, though auroral activity can increase.
General Propagation Notes
Often strongest after sunset and overnight. Less dependent on high solar flux than upper HF.
Often useful day and night, with changing paths as daylight moves around the globe.
Higher solar activity can create excellent long-distance openings, especially during daylight.
Sporadic-E, tropospheric enhancement and other modes can produce sudden long-distance openings.
Normally line-of-sight, but temperature inversions, ducting, aurora and Sporadic-E can extend range.
Antenna height and terrain matter greatly. Tropospheric enhancement can occasionally extend paths well beyond normal range.
LOCAL RADIO CONDITIONS
Propagation Outlook — ZIP 44134
Parma, Ohio area • live space-weather and local weather inputs
10 Meters
--Waiting for current solar conditions.
6 Meters
--Waiting for current conditions.
2 Meters
--Waiting for local weather conditions.
70 Centimeters
--Waiting for local weather conditions.
The VHF/UHF outlook is a local indicator based on surface weather near ZIP 44134. It can suggest conditions favorable for tropospheric enhancement, but it is not a ducting forecast and cannot guarantee an opening.