Solar outages can be accurately predicted and occur when the sun passes within the field of view of an antenna. See Rain Outage.
As a satellite receiver antenna is pointed towards the satellite, it also points at the hot sun. This results in thermal noise being picked up by the antenna.
The loss of reception that occurs when the sun is positioned directly behind a target satellite. When this occurs, solar noise drowns out the satellite signal and reception is lost.
Solar outages occur when a satellite dish is looking at a satellite, and the sun passes behind the satellite and within the field of view of the dish antenna. Solar outages occur during the spring and fall as the sun moves up and down the sky during the equinox. The outages only last a few minutes for a few days a year.
Outage that occurs when the sun passes behind or near the satellite and within the field of view of the antenna. This field of view is usually wider than the beam width. Timing of solar outages can be exactly predicted for each site.
This is an outage that occurs when the sun moves behind the transmitting satellite within the view of your satellite dish. This type of outage only happens a few minutes a year.
Solar outages occur when an antenna is looking at a satellite, and the sun passes behind or near the satellite and within the field of view of the antenna. The field of view is usually wider than the beamwidth. Solar outages can be exactly predicted as to the timing of each site.
Interference occurring when the sun passes behind or near a satellite and within the field of view of the antenna. Solar outages can be exactly predicted.
Solar outages occur when an antenna is looking at a satellite, and the sun passes behind or near the satellite and within the field of view of the antenna. Solar outages occur each year at the beginning of spring and fall and can be exactly predicted as to the timing for each site.
An outage that occurs when the sun passes near or behind the satellite and within the field of view of the antenna. This field of view is usually wider than the beamwidth.