Changeset 11119 in ntrip
- Timestamp:
- Oct 22, 2026, 6:20:09 PM (8 hours ago)
- Location:
- trunk/BNC/src
- Files:
-
- 2 edited
-
bnchelp.html (modified) (2 diffs)
-
ssrQc.cpp (modified) (3 diffs)
Legend:
- Unmodified
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trunk/BNC/src/bnchelp.html
r11117 r11119 5134 5134 <li>the code bias signals provided, satellites without code biases of the reference signals (default GPS C1W/C2W, 5135 5135 GLONASS C1P/C2P, Galileo C1C/C5Q, BDS C2I/C6I, QZSS C1C/C2L, SBAS C1C/C5Q; as in the combination, see option 5136 'Reference Signals' in <a href=#combirefsig>section 2.14.1.7</a>), and the standard deviation and maximum of the 5137 ionosphere-free combination B_IF of the reference signal biases. A B_IF varying between the satellites is 5138 legitimate if the clocks are estimated with other signals, but must then be consistent with the clocks 5139 (see section 'Combination'),</li> 5136 'Reference Signals' in <a href=#combirefsig>section 2.14.1.7</a>), and the standard deviation, the median of the 5137 absolute values and the maximum (with the satellite) of the ionosphere-free combination B_IF of the reference 5138 signal biases. A B_IF varying between the satellites is legitimate if the clocks are estimated with other 5139 signals, but must then be consistent with the clocks (see section 'Combination'). A median close to zero with a 5140 large standard deviation points to single satellites with inconsistent biases (the satellite with the maximum), 5141 a large median to clocks estimated with other signals,</li> 5140 5142 <li>the code bias check: the DCBs of the stream, i.e. the differences of its code biases to the first reference 5141 5143 signal (or to another common signal, if the stream lacks it), are compared with … … 5186 5188 G corrections referring to an IOD of no received broadcast ephemeris: G10(94) G22(94) G29(94) 5187 5189 G code bias signals: 1C 1P 1W 2L 2P 2S 2W 5Q 5188 G ionosphere-free combination B_IF of the reference signal biases: std. dev. 0.58 6m, max |B_IF| 2.058 m(32 satellites)5190 G ionosphere-free combination B_IF of the reference signal biases: std. dev. 0.585 m, median |B_IF| 0.297 m, max |B_IF| 2.032 m (G19) (32 satellites) 5189 5191 G largest orbit corrections: radial 1.06 m (G11), along/cross 2.05 m (G11) 5190 5192 </pre> -
trunk/BNC/src/ssrQc.cpp
r11117 r11119 1279 1279 QString maxRadialPrn, maxAlongCrossPrn; 1280 1280 QVector<double> biasIF; 1281 double maxBiasIF = 0.0; 1282 QString biasIFPrn; 1281 1283 const QSet<QString>& ephs = ephSats[sys]; 1282 1284 for (int type = ORB; type <= PBIAS; type++) { … … 1321 1323 if (stat.refBiasOK) { 1322 1324 biasIF.push_back(stat.biasIF); 1325 if (biasIFPrn.isEmpty() || fabs(stat.biasIF) > maxBiasIF) { 1326 maxBiasIF = fabs(stat.biasIF); 1327 biasIFPrn = prn; 1328 } 1323 1329 } 1324 1330 if (stat.numPB) { … … 1373 1379 double var = 0.0; 1374 1380 for (double bb : biasIF) var += (bb - mean) * (bb - mean) / biasIF.size(); 1375 double maxAbs = max(fabs(*std::min_element(biasIF.begin(), biasIF.end())), 1376 fabs(*std::max_element(biasIF.begin(), biasIF.end()))); 1381 // the median shows whether the clocks refer to other signals (all 1382 // satellites) or single satellites have inconsistent biases 1383 QVector<double> absIF; 1384 for (double bb : biasIF) absIF << fabs(bb); 1377 1385 lines << QString("ionosphere-free combination B_IF of the reference signal biases: " 1378 "std. dev. %1 m, max |B_IF| %2 m (%3 satellites)") 1379 .arg(sqrt(var), 0, 'f', 3).arg(maxAbs, 0, 'f', 3).arg(biasIF.size()); 1386 "std. dev. %1 m, median |B_IF| %2 m, max |B_IF| %3 m (%4) (%5 satellites)") 1387 .arg(sqrt(var), 0, 'f', 3).arg(median(absIF), 0, 'f', 3).arg(maxBiasIF, 0, 'f', 3) 1388 .arg(biasIFPrn).arg(biasIF.size()); 1380 1389 } 1381 1390 }
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