Signal strength and picture quality resolved...
The science confirms my claims. Granted, it was hard to find. Most things written about the subject are written in terms of upper performance limits rather than lower limits; of digital superiority over analog, not that it has the same obstacles to overcome.
Digital is described as more "robust" to the analog influences like ghosting and interference. More robust, not immune.
Prior to the advent of HDTV, we didn't have many choices of picture quality. We didn't need a very discriminating eye to see how superior digital was to analog. In the early days of satellite it was easy to align a dish. All you had to hit was one strong satellite. Early systems had less noise to deal with, also, and before long the digital myth became digital mantra - "Digital is all or nothing", "Signal strength won't effect picture quality", and a host of similar, but incorrect statements.
Today, we have not one strong satellite (119), but we've added 110 (weaker) and, with the advent of HDTV, have added not one but two much weaker satellites. The 129 and 118.7 are about 80% of the strength of 119/110.
Today, we put in much larger systems with multiple receivers, switches, and multi-sat dishes. Technology within our homes and neighborhoods has exploded and wireless technology is everywhere. Today, we put in systems that have much greater noise to overcome.
Multi-sat dishes continue to be a challenge for many technicians with the weak satellite peaking required for the HD.
These factors combine to cause a significant number of systems left with marginal HD signal, and resulting poor quality.
Here's some science for you.
In terms of digital receiver operating specifications, there are a couple of descriptive terms that I found particularly interesting.
The point that we call "signal lock" has a name. It actually has two, both very descriptive. It is called either, the "failure point" or FP by DVB standards, and the ATSC calls it the "Threshold of Visibility or TOV.
It has a definition, too. It is defined in a bit error rate and it is defined in number of corrupted transport packets per time frame.
Failure Point (FP) - In digital receiver reception (DVB-T), the failure point is defined as the lowest rate it is practical to observe requiring an observation interval of about 1.5 minutes, or an average of two correctable transport packets per ten seconds. ATSC defines the failure point as the threshold of visibility (TOV).
With digital receivers this is the beginning. We have a signal but we're only getting enough information for a corrupted picture.
We have to reach the QEF condition. What is the QEF condition? It is called the "Quasi-Error Free" condition. Another descriptive term with "Quasi" meaning "semi" or "Sort-of", error free condition.
With bit error rates we aren't required to remove all of the errors, there are awesome error correction measures in the digital receiver. We have to reduce the bit error rate to a manageable level.
QEF - Quasi Error Free The QEF point is the error rate where the reed solomon code reaches the limit of its correction ability for white noise degradation. Strictly, the QEF is defined as 1 uncorrectable transport packet per hour; or bit error ratio of 2E-4 after the Viterbi decoder for ATSC and DVB-T. For cable TV the system FEC is optimized for quasi error free operation at a threshold output error event rate of one error event per 15 minutes.
As you increase signal you reduce the bit error rate to where you have enough uncorrupted information to produce the "perfect" digital picture. (The QEF condition)
In Dish terms (old meter) lets say that the FP is 50. The QEF is definitely achieved by 70. (Of course, it is impossible to have one reading for everyone due to differences in systems.)
But, what if we stopped there at the QEF point? If we did, picture would be great until
any additional noise or signal drop came along.
The amount of signal that you have, above the QEF point, is what is available to counteract weather and noise influences. If you're only a few points above the QEF, a small rain shower would put you under the QEF, and could compromise the picture even though you still have lock.
Now consider again the weak HD satellites. They don't have from 70 to 115 signal strength (45 points of signal strength) to overcome noise like 119 does. The HD satellites are not even capable of receiving as much noise fighting signal in the first place. They might have from 70 to 85 signal strength to work with, or 15 points. A storm only has to lower the signal by 16 points to dip below the QEF. If your signal isn't maxed, it won't take much at all to dip below the QEF! This is why it becomes CRITICAL to max the HD signals!
You may think this isn't a problem, but the poll suggests that over 20% of installers have experienced systems in the "below QEF" condition. That alone suggests that the potential of customers existing below QEF (especially now in terms of HD), is quite large indeed.
Due to the poor skills and understanding of some technicians, and other reasons mentioned above, many are left complaining about Dish's poor picture quality. My experience says that Dish quality is second, only slightly, to good OTA. I don't believe that there is any reason why people should be complaining about quality, unless they've checked everything else and when they ask if it could be their low signal strength, they are told "No."
All the science and references are here:
Signal and HD
And to all who contributed to the thread, thanks for playing!
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