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Dark Skies are a Universal Resource. So Are Quiet Skies
| Content Provider | Semantic Scholar |
|---|---|
| Author | Maddalena, Ronald J. |
| Copyright Year | 2008 |
| Abstract | The QS Detector can be operated in wide-band mode and narrow-band mode. When in wide-band mode, the detector acts much like a optical light meter in that it reports the total amount of power between 800 and 1700 MHz. When in narrow-band mode the detector can be tuned in frequency. This allows the user to determine the frequency of an RFI signal to within 5 MHz. The frequency of an RFI source is a clue to what it is. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://www.gb.nrao.edu/~sheather/qsposter.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |