| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50 | 622 | 25 | 312 | 9.88 | 268.34 | -9.83 | 57.95 | 0.1978 | 848.2 | 282.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-02 17:51:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 4 | 6.96 | 276.86 | -1.31 | 24.62 | 0.0549 | 856.0 | 745.2 | |
| 0 | 4 | 0 | 2 | 5.92 | 275.78 | -2.39 | 52.79 | 0.0524 | 905.0 | 770.0 | |
| 0 | 4 | 0 | 2 | 6.77 | 275.66 | -2.52 | 43.25 | 0.0639 | 582.0 | 516.3 | |
| 0 | 8 | 0 | 4 | 6.53 | 274.42 | -3.75 | 56.97 | 0.0780 | 875.0 | 838.3 | |
| 0 | 3 | 0 | 2 | 9.73 | 273.25 | -4.92 | 40.77 | 0.1301 | 475.0 | 544.0 | |
| 0 | 4 | 0 | 2 | 8.83 | 272.99 | -5.18 | 47.22 | 0.1222 | 812.0 | 671.0 | |
| 0 | 15 | 0 | 8 | 6.60 | 272.78 | -5.39 | 64.92 | 0.1035 | 1283.0 | 1011.8 | |
| 0 | 7 | 0 | 3 | 10.38 | 272.61 | -5.56 | 41.04 | 0.1458 | 700.0 | 629.8 | |
| 0 | 8 | 0 | 4 | 8.64 | 272.60 | -5.57 | 50.45 | 0.1250 | 887.0 | 780.2 | |
| 0 | 4 | 0 | 2 | 6.40 | 272.44 | -5.74 | 67.92 | 0.1077 | 628.0 | 503.5 | |
| 0 | 4 | 0 | 2 | 9.33 | 272.16 | -6.01 | 48.53 | 0.1386 | 636.0 | 525.9 | |
| 0 | 9 | 0 | 4 | 7.09 | 272.19 | -5.98 | 63.12 | 0.1164 | 866.0 | 610.7 | |
| 2 | 51 | 1 | 25 | 7.56 | 272.03 | -6.14 | 60.32 | 0.1226 | 1382.5 | 733.5 | |
| 0 | 4 | 0 | 2 | 8.71 | 271.94 | -6.24 | 53.11 | 0.1349 | 741.0 | 670.7 | |
| 0 | 10 | 0 | 5 | 11.38 | 271.84 | -6.33 | 40.41 | 0.1675 | 899.0 | 739.5 | |
| 0 | -13 | 0 | -13 | 7.44 | 271.80 | -6.37 | 62.04 | 0.1252 | 1186.0 | 999999 | |
| 0 | 7 | 0 | 3 | 9.06 | 271.77 | -6.40 | 51.80 | 0.1407 | 1021.0 | 791.5 | |
| 0 | 4 | 0 | 2 | 12.31 | 271.66 | -6.51 | 37.75 | 0.1817 | 926.0 | 773.7 | |
| 0 | 11 | 0 | 5 | 6.32 | 271.62 | -6.55 | 71.05 | 0.1205 | -828.0 | -561.7 | |
| 0 | 9 | 0 | 4 | 8.17 | 271.36 | -6.81 | 58.78 | 0.1380 | 836.0 | 825.2 | |
| 0 | 9 | 0 | 5 | 8.44 | 271.27 | -6.90 | 57.43 | 0.1416 | 989.0 | 802.1 | |
| 0 | 5 | 0 | 2 | 8.94 | 271.11 | -7.06 | 55.14 | 0.1487 | 648.0 | 589.5 | |
| 0 | 5 | 0 | 2 | 8.90 | 270.79 | -7.38 | 56.51 | 0.1528 | 735.0 | 648.8 | |
| 0 | 7 | 0 | 3 | 9.36 | 270.51 | -7.66 | 55.03 | 0.1613 | 581.0 | 522.7 | |
| 0 | 10 | 0 | 5 | 12.26 | 270.16 | -8.01 | 43.74 | 0.1980 | 547.0 | 561.6 | |
| 4 | 10 | 2 | 5 | 6.35 | 270.25 | -7.92 | 73.86 | 0.1432 | -958.5 | -622.4 | |
| 4 | 233 | 2 | 118 | 9.54 | 269.68 | -8.49 | 56.79 | 0.1749 | 1264.0 | 701.0 | |
| 6 | -27 | 3 | -27 | 10.08 | 269.51 | -8.67 | 54.77 | 0.1824 | 1660.4 | 999999 | |
| 6 | -27 | 3 | -27 | 9.65 | 269.40 | -8.77 | 57.07 | 0.1800 | 1596.5 | 999999 | |
| 8 | -27 | 4 | -27 | 10.00 | 269.03 | -9.14 | 56.53 | 0.1884 | 1459.8 | 999999 | |
| 3 | -27 | 2 | -27 | 9.84 | 268.80 | -9.37 | 57.88 | 0.1903 | 1735.2 | 999999 | |
| 6 | -27 | 3 | -27 | 9.99 | 268.48 | -9.69 | 58.05 | 0.1963 | 1215.1 | 999999 | |
| 5 | -27 | 2 | -27 | 9.83 | 268.13 | -10.04 | 59.62 | 0.2001 | 1173.7 | 999999 | |
| 0 | 4 | 0 | 2 | 6.63 | 268.05 | -10.12 | 75.55 | 0.1811 | -720.0 | -502.5 | |
| 3 | -27 | 2 | -27 | 9.79 | 267.69 | -10.48 | 60.83 | 0.2062 | 1112.3 | 999999 | |
| 0 | 4 | 0 | 2 | 8.85 | 266.61 | -11.56 | 67.03 | 0.2161 | 586.0 | 577.7 | |
| 0 | 3 | 0 | 2 | 9.70 | 266.58 | -11.59 | 63.51 | 0.2223 | 292.0 | 208.4 | |
| 3 | 25 | 1 | 13 | 12.19 | 264.87 | -13.30 | 57.67 | 0.2674 | -1204.0 | -834.1 | |
| 0 | 5 | 0 | 2 | 9.17 | 264.88 | -13.29 | 68.37 | 0.2452 | -752.0 | -616.2 | |
| 0 | 5 | 0 | 2 | 13.15 | 264.33 | -13.84 | 55.66 | 0.2834 | -481.0 | -377.5 | |
| 0 | 2 | 0 | 1 | 12.72 | 264.15 | -14.02 | 57.29 | 0.2821 | -558.0 | -545.8 | |
| 0 | 3 | 0 | 2 | 11.98 | 264.07 | -14.10 | 59.75 | 0.2772 | -914.0 | -832.8 | |
| 0 | 4 | 0 | 2 | 12.45 | 264.00 | -14.17 | 58.39 | 0.2819 | -825.0 | -659.1 | |
| 0 | 4 | 0 | 2 | 11.75 | 263.92 | -14.25 | 60.75 | 0.2775 | -873.0 | -705.2 | |
| 0 | 5 | 0 | 2 | 13.22 | 263.80 | -14.38 | 56.41 | 0.2915 | -429.0 | -369.5 | |
| 0 | 19 | 0 | 10 | 12.93 | 262.87 | -15.30 | 58.79 | 0.3020 | -1055.0 | -883.8 | |
| 0 | 4 | 0 | 2 | 12.43 | 262.86 | -15.31 | 60.30 | 0.2982 | -863.0 | -788.9 | |
| 0 | 6 | 0 | 3 | 11.84 | 262.78 | -15.40 | 62.20 | 0.2951 | -1206.0 | -1014.0 | |
| 0 | 21 | 0 | 11 | 12.76 | 262.10 | -16.07 | 60.43 | 0.3117 | -897.0 | -724.9 | |
| 0 | 6 | 0 | 3 | 11.00 | 261.52 | -16.65 | 66.40 | 0.3084 | -814.0 | -682.4 | |
| 0 | 9 | 0 | 5 | 8.41 | 261.65 | -16.52 | 74.52 | 0.2932 | -859.0 | -773.2 | |
| 0 | 10 | 0 | 5 | 13.83 | 260.96 | -17.22 | 59.11 | 0.3364 | -951.0 | -785.7 | |
| 0 | 4 | 0 | 2 | 14.10 | 260.73 | -17.44 | 58.72 | 0.3417 | -867.0 | -777.3 | |
| 0 | 12 | 0 | 7 | 12.38 | 260.65 | -17.52 | 63.43 | 0.3303 | -704.0 | -635.1 | |
| 0 | 6 | 0 | 3 | 11.85 | 259.52 | -18.65 | 66.15 | 0.3437 | -534.0 | -570.6 | |
| 0 | 8 | 0 | 4 | 13.72 | 259.21 | -18.96 | 61.61 | 0.3604 | -597.0 | -560.9 | |
| 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. | |