| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.71 | 149.11 | 17.86 | 74.56 | -9.94 | 358.34 | 6.30 | 240.70 | 0.1377 | 588.0 | 413.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.57 | -13.08 | 0.52 | 8.47 | 234.21 | 0.1778 | 856.0 | 750.5 | |
| 0.00 | 2.17 | 0.00 | 1.08 | -6.14 | 0.17 | 8.13 | 277.11 | 0.1423 | 1074.0 | 881.5 | |
| 16.38 | 62.67 | 8.20 | 31.39 | -9.92 | 0.12 | 8.08 | 250.72 | 0.1473 | 1374.1 | 518.7 | |
| 0.00 | 3.90 | 0.00 | 1.95 | -8.28 | 360.00 | 7.95 | 261.75 | 0.1390 | 1067.0 | 894.2 | |
| 0.00 | 3.64 | 0.00 | 1.82 | -7.98 | 359.99 | 7.95 | 263.89 | 0.1383 | 1189.0 | 979.6 | |
| 0.00 | 3.12 | 0.00 | 1.56 | -7.51 | 359.98 | 7.94 | 267.35 | 0.1377 | 902.0 | 733.8 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -6.26 | 359.93 | 7.89 | 276.47 | 0.1379 | 769.0 | 697.2 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -7.66 | 359.71 | 7.67 | 266.13 | 0.1331 | 1047.0 | 919.6 | |
| 18.29 | 21.85 | 9.14 | 10.92 | -9.33 | 359.59 | 7.55 | 253.65 | 0.1357 | 1159.7 | 730.6 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -7.51 | 359.56 | 7.51 | 267.20 | 0.1304 | 871.0 | 698.9 | |
| 0.00 | 2.25 | 0.00 | 1.13 | -7.67 | 359.38 | 7.33 | 265.96 | 0.1274 | 986.0 | 857.2 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -7.04 | 359.13 | 7.08 | 270.93 | 0.1230 | 942.0 | 729.4 | |
| 0.00 | 3.99 | 0.00 | 1.99 | -7.55 | 359.10 | 7.06 | 266.78 | 0.1226 | 1029.0 | 956.0 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -14.21 | 358.95 | 6.90 | 223.52 | 0.1700 | 800.0 | 709.9 | |
| 1.04 | 2.51 | 0.52 | 1.25 | -8.51 | 358.73 | 6.68 | 258.48 | 0.1180 | 1064.2 | 899.6 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -8.43 | 358.27 | 6.23 | 258.47 | 0.1100 | 987.0 | 764.5 | |
| 0.00 | 4.25 | 0.00 | 2.12 | -8.22 | 358.24 | 6.19 | 260.30 | 0.1088 | 849.0 | 705.3 | |
| 0.00 | 2.17 | 0.00 | 1.08 | -6.40 | 358.00 | 5.96 | 277.42 | 0.1045 | 830.0 | 687.1 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -6.58 | 358.01 | 5.96 | 275.71 | 0.1042 | 965.0 | 735.5 | |
| 0.00 | 1.91 | 0.00 | 0.95 | -13.64 | 356.53 | 4.49 | 214.10 | 0.1362 | 881.0 | 599.7 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -13.34 | 356.25 | 4.20 | 213.68 | 0.1292 | 878.0 | 784.0 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -11.63 | 356.22 | 4.18 | 222.67 | 0.1058 | 921.0 | 715.9 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -14.27 | 355.56 | 3.51 | 205.74 | 0.1373 | 779.0 | 533.4 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -15.84 | 355.36 | 3.32 | 200.35 | 0.1609 | -820.0 | -639.7 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -13.94 | 355.21 | 3.17 | 204.56 | 0.1297 | 1060.0 | 873.1 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -15.69 | 354.50 | 2.45 | 195.59 | 0.1539 | -950.0 | -785.3 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -15.96 | 354.22 | 2.17 | 193.48 | 0.1572 | -972.0 | -761.6 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -13.56 | 352.12 | 0.07 | 180.62 | 0.1111 | -981.0 | -743.2 | |
| 0.00 | 0.87 | 0.00 | 0.43 | -15.53 | 349.86 | -2.19 | 165.76 | 0.1501 | -733.0 | -623.5 | |
| 0.00 | 2.60 | 0.00 | 1.29 | -9.13 | 349.59 | -2.46 | 128.48 | 0.0543 | -875.0 | -717.4 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -15.83 | 349.48 | -2.56 | 164.01 | 0.1568 | -900.0 | -721.7 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -9.49 | 349.52 | -2.52 | 132.60 | 0.0592 | -931.0 | -849.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -13.43 | 349.27 | -2.78 | 156.52 | 0.1188 | -753.0 | -633.2 | |
| 0.00 | 1.65 | 0.00 | 0.83 | -16.07 | 348.46 | -3.59 | 158.68 | 0.1662 | -922.0 | -764.4 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -12.93 | 347.01 | -5.03 | 139.48 | 0.1323 | -883.0 | -674.9 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -13.34 | 346.30 | -5.75 | 137.76 | 0.1457 | -977.0 | -793.9 | |
| 0.00 | 1.65 | 0.00 | 0.82 | -10.25 | 345.57 | -6.47 | 115.89 | 0.1239 | -910.0 | -715.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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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. |
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| 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. | |