SOHO MDI 2000-09-03 17:03:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 163 | 882 | 84 | 445 | 13.28 | 357.69 | 7.60 | 309.33 | 0.1677 | 788.3 | 290.8 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-09-03 17:03:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 73 | 2 | 37 | 12.93 | 2.53 | 12.44 | 295.92 | 0.2345 | 1324.2 | 787.9 | |
| 0 | 5 | 0 | 2 | 11.71 | 2.48 | 12.38 | 291.06 | 0.2260 | 964.0 | 725.8 | |
| 5 | -1 | 3 | -1 | 13.22 | 2.34 | 12.25 | 297.35 | 0.2336 | 1210.3 | 999999 | |
| 9 | -1 | 5 | -1 | 12.74 | 2.28 | 12.18 | 295.60 | 0.2293 | 1523.0 | 999999 | |
| 0 | 4 | 0 | 2 | 13.85 | 2.33 | 12.24 | 299.78 | 0.2383 | 553.0 | 481.4 | |
| 6 | -1 | 3 | -1 | 12.99 | 2.04 | 11.95 | 296.99 | 0.2274 | 1486.5 | 999999 | |
| 0 | 6 | 0 | 3 | 12.76 | 1.66 | 11.57 | 296.76 | 0.2201 | 1016.0 | 832.1 | |
| 0 | 10 | 0 | 5 | 11.62 | 1.49 | 11.40 | 292.15 | 0.2099 | 1058.0 | 800.5 | |
| 0 | 5 | 0 | 3 | 15.13 | 1.49 | 11.40 | 306.21 | 0.2376 | 595.0 | 529.3 | |
| 0 | 17 | 0 | 9 | 13.05 | 1.22 | 11.13 | 298.81 | 0.2156 | 461.0 | 686.6 | |
| 8 | 383 | 4 | 194 | 12.66 | 0.67 | 10.58 | 298.33 | 0.2045 | 1315.7 | 726.8 | |
| 12 | -11 | 6 | -11 | 13.19 | 0.08 | 9.99 | 301.99 | 0.2000 | 1572.4 | 999999 | |
| 49 | -11 | 25 | -11 | 13.62 | 0.10 | 10.01 | 303.79 | 0.2041 | 2100.0 | 999999 | |
| -13 | -11 | -13 | -11 | 13.87 | 359.70 | 9.61 | 305.86 | 0.2009 | 999999 | 999999 | |
| 0 | 3 | 0 | 2 | 11.27 | 359.56 | 9.47 | 294.03 | 0.1775 | -464.0 | -400.7 | |
| -13 | -11 | -13 | -11 | 13.55 | 359.65 | 9.55 | 304.68 | 0.1971 | 999999 | 999999 | |
| 5 | 55 | 2 | 28 | 12.47 | 358.59 | 8.50 | 302.66 | 0.1721 | 792.2 | 757.3 | |
| 0 | 4 | 0 | 2 | 11.60 | 358.56 | 8.47 | 298.22 | 0.1645 | -403.0 | -333.7 | |
| 3 | -17 | 2 | -17 | 12.08 | 358.37 | 8.28 | 301.30 | 0.1656 | -148.0 | 999999 | |
| 4 | -17 | 2 | -17 | 12.36 | 358.22 | 8.13 | 303.22 | 0.1658 | 1120.1 | 999999 | |
| 0 | 4 | 0 | 2 | 13.90 | 358.15 | 8.06 | 310.72 | 0.1803 | 752.0 | 614.2 | |
| 15 | 56 | 8 | 28 | 13.35 | 357.93 | 7.83 | 309.04 | 0.1715 | 1491.5 | 800.7 | |
| 3 | -17 | 1 | -17 | 12.52 | 357.82 | 7.73 | 305.37 | 0.1617 | 1272.6 | 999999 | |
| 0 | 2 | 0 | 1 | 14.22 | 357.87 | 7.78 | 313.05 | 0.1804 | 700.0 | 566.8 | |
| 0 | 6 | 0 | 3 | 12.42 | 356.68 | 6.59 | 309.11 | 0.1451 | 458.0 | 426.9 | |
| 0 | 6 | 0 | 3 | 12.09 | 355.22 | 5.13 | 314.17 | 0.1225 | -437.0 | -368.1 | |
| 0 | 4 | 0 | 2 | 13.15 | 354.92 | 4.83 | 321.60 | 0.1326 | -633.0 | -444.2 | |
| 0 | 6 | 0 | 3 | 13.87 | 354.57 | 4.48 | 326.78 | 0.1390 | -731.0 | -539.7 | |
| 3 | 18 | 2 | 9 | 13.52 | 353.76 | 3.66 | 330.45 | 0.1265 | -1118.3 | -964.1 | |
| 0 | 8 | 0 | 4 | 13.64 | 353.11 | 3.02 | 335.38 | 0.1234 | -812.0 | -765.0 | |
| 0 | 8 | 0 | 4 | 14.04 | 352.55 | 2.46 | 340.66 | 0.1261 | -849.0 | -800.2 | |
| 0 | 3 | 0 | 1 | 13.84 | 352.39 | 2.29 | 341.34 | 0.1220 | -990.0 | -941.5 | |
| 0 | 9 | 0 | 4 | 13.33 | 352.22 | 2.13 | 341.21 | 0.1126 | -943.0 | -874.3 | |
| 6 | 144 | 3 | 72 | 12.70 | 352.13 | 2.04 | 339.95 | 0.1018 | -1247.3 | -860.0 | |
| 0 | 19 | 0 | 10 | 14.00 | 351.94 | 1.85 | 345.11 | 0.1224 | -1355.0 | -952.6 | |
| 0 | 9 | 0 | 4 | 14.48 | 351.87 | 1.77 | 346.63 | 0.1301 | -914.0 | -803.2 | |
| 10 | -34 | 5 | -34 | 13.14 | 351.73 | 1.64 | 344.81 | 0.1069 | -1554.5 | 999999 | |
| 7 | -34 | 4 | -34 | 13.26 | 351.25 | 1.16 | 349.36 | 0.1071 | -1577.5 | 999999 | |
| 14 | -34 | 7 | -34 | 13.18 | 350.93 | 0.84 | 352.18 | 0.1049 | -1652.9 | 999999 | |
| -39 | -34 | -39 | -34 | 13.06 | 350.69 | 0.59 | 354.31 | 0.1023 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | 14.92 | 349.52 | -0.58 | 4.18 | 0.1345 | -769.0 | -750.8 | |
| 0 | 5 | 0 | 3 | 14.24 | 349.36 | -0.74 | 5.85 | 0.1231 | -802.0 | -649.3 | |
| 0 | 5 | 0 | 2 | 14.08 | 347.25 | -2.84 | 21.97 | 0.1291 | -502.0 | -403.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |