| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.71 | 115.55 | 24.13 | 72.92 | 14.52 | 56.35 | 38.11 | 284.96 | 0.6196 | -104.0 | -192.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.95 | 11.54 | 60.10 | 41.86 | 279.66 | 0.6656 | -816.0 | -722.8 | |
| 6.75 | 10.62 | 4.49 | 7.06 | 13.77 | 60.27 | 42.02 | 282.99 | 0.6696 | -766.6 | -416.5 | |
| 0.00 | 0.99 | 0.00 | 0.66 | 16.16 | 59.74 | 41.50 | 286.64 | 0.6666 | -453.0 | -422.8 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 16.39 | 59.55 | 41.31 | 287.03 | 0.6646 | -572.0 | -498.5 | |
| 3.15 | 56.06 | 2.04 | 36.19 | 14.27 | 58.54 | 40.30 | 284.01 | 0.6483 | -596.0 | -595.3 | |
| 8.46 | -5.00 | 5.47 | -5.00 | 14.26 | 58.33 | 40.09 | 284.02 | 0.6456 | -913.8 | 999999 | |
| 1.44 | 2.88 | 0.93 | 1.87 | 14.71 | 58.43 | 40.19 | 284.70 | 0.6476 | -700.8 | -585.4 | |
| 0.00 | 0.81 | 0.00 | 0.52 | 13.38 | 58.15 | 39.91 | 282.68 | 0.6421 | -621.0 | -539.7 | |
| 10.62 | -5.00 | 6.86 | -5.00 | 13.96 | 58.23 | 39.99 | 283.57 | 0.6438 | -898.7 | 999999 | |
| 0.81 | 2.34 | 0.52 | 1.50 | 13.81 | 57.71 | 39.47 | 283.43 | 0.6369 | -905.6 | -755.9 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 18.27 | 58.67 | 40.43 | 290.05 | 0.6578 | -503.0 | -413.9 | |
| 0.00 | 1.08 | 0.00 | 0.69 | 16.99 | 57.01 | 38.76 | 288.55 | 0.6339 | -661.0 | -555.1 | |
| 0.00 | 2.07 | 0.00 | 1.32 | 17.37 | 56.94 | 38.70 | 289.15 | 0.6339 | -634.0 | -565.1 | |
| 0.00 | 1.35 | 0.00 | 0.83 | 14.50 | 54.16 | 35.92 | 285.25 | 0.5908 | 632.0 | 531.3 | |
| 0.00 | 1.53 | 0.00 | 0.93 | 14.55 | 53.36 | 35.12 | 285.54 | 0.5801 | 458.0 | 376.2 | |
| 0.00 | 2.79 | 0.00 | 1.69 | 14.43 | 52.95 | 34.71 | 285.43 | 0.5742 | 797.0 | 611.0 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 14.81 | 52.83 | 34.59 | 286.11 | 0.5734 | 562.0 | 457.9 | |
| 0.63 | 2.25 | 0.38 | 1.35 | 14.71 | 52.43 | 34.19 | 286.06 | 0.5677 | 794.9 | 592.9 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 14.63 | 51.25 | 33.01 | 286.27 | 0.5512 | 620.0 | 572.7 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 16.85 | 51.36 | 33.12 | 290.16 | 0.5591 | 567.0 | 422.5 | |
| 0.36 | 1.80 | 0.21 | 1.07 | 16.28 | 51.06 | 32.82 | 289.27 | 0.5532 | 619.0 | 492.6 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 16.20 | 50.89 | 32.65 | 289.19 | 0.5507 | 599.0 | 472.1 | |
| 3.96 | 8.73 | 2.33 | 5.14 | 14.98 | 50.63 | 32.39 | 287.09 | 0.5435 | 848.8 | 679.2 | |
| 1.53 | -23.00 | 0.90 | -23.00 | 15.08 | 50.47 | 32.23 | 287.33 | 0.5415 | 900.4 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.75 | 16.46 | 50.68 | 32.44 | 289.73 | 0.5486 | 705.0 | 546.9 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 16.25 | 50.60 | 32.36 | 289.39 | 0.5468 | 516.0 | 555.1 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 18.25 | 50.85 | 32.61 | 292.81 | 0.5573 | 435.0 | 329.0 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 15.50 | 50.20 | 31.96 | 288.19 | 0.5390 | 699.0 | 567.9 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 15.93 | 49.72 | 31.48 | 289.16 | 0.5337 | 252.0 | 294.8 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 19.99 | 49.98 | 31.74 | 296.26 | 0.5533 | 581.0 | 562.5 | |
| 0.00 | 0.27 | 0.00 | 0.16 | 20.07 | 49.69 | 31.45 | 296.55 | 0.5500 | 536.0 | 551.0 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 13.35 | 48.11 | 29.87 | 284.84 | 0.5033 | 655.0 | 570.4 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 12.49 | 47.64 | 29.40 | 283.27 | 0.4944 | 784.0 | 548.8 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 14.23 | 47.23 | 28.99 | 286.90 | 0.4930 | 431.0 | 413.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 10.33 | 46.55 | 28.31 | 279.06 | 0.4743 | 625.0 | 527.5 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 14.38 | 46.86 | 28.62 | 287.34 | 0.4880 | 696.0 | 593.1 | |
| 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. | |