| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 191.34 | 879.76 | 178.79 | 826.78 | 15.16 | 261.01 | 58.67 | 283.72 | 0.8496 | -47.8 | -115.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 179.00 | 0.88 | 192.66 | 12.88 | 266.68 | 64.34 | 281.04 | 0.8971 | -338.7 | -183.1 | |
| 1.76 | -1.00 | 1.96 | -1.00 | 13.16 | 266.60 | 64.26 | 281.36 | 0.8965 | -105.4 | 999999 | |
| 3.00 | -1.00 | 3.29 | -1.00 | 13.32 | 266.25 | 63.91 | 281.53 | 0.8938 | -368.1 | 999999 | |
| 16.83 | -1.00 | 18.12 | -1.00 | 13.59 | 265.75 | 63.41 | 281.82 | 0.8899 | -665.3 | 999999 | |
| 4.32 | -1.00 | 4.58 | -1.00 | 13.98 | 265.25 | 62.91 | 282.26 | 0.8860 | -651.6 | 999999 | |
| 2.12 | -1.00 | 2.22 | -1.00 | 13.64 | 264.95 | 62.61 | 281.87 | 0.8836 | -816.5 | 999999 | |
| 6.52 | -1.00 | 6.83 | -1.00 | 13.99 | 264.85 | 62.51 | 282.27 | 0.8828 | -868.0 | 999999 | |
| 0.00 | 4.41 | 0.00 | 4.34 | 13.59 | 262.83 | 60.49 | 281.80 | 0.8662 | -630.0 | -551.3 | |
| 31.99 | 278.86 | 31.02 | 266.10 | 15.15 | 262.28 | 59.94 | 283.62 | 0.8616 | -898.6 | -408.8 | |
| 12.96 | -9.00 | 12.15 | -9.00 | 14.81 | 261.08 | 58.74 | 283.25 | 0.8511 | 153.5 | 999999 | |
| 11.72 | -9.00 | 11.13 | -9.00 | 15.84 | 261.55 | 59.21 | 284.45 | 0.8555 | -829.8 | 999999 | |
| 7.93 | -9.00 | 7.49 | -9.00 | 15.31 | 261.30 | 58.96 | 283.83 | 0.8532 | -1126.3 | 999999 | |
| 0.00 | 1.67 | 0.00 | 1.61 | 16.52 | 261.89 | 59.55 | 285.23 | 0.8586 | -156.0 | -112.3 | |
| 0.00 | 0.44 | 0.00 | 0.42 | 16.72 | 261.74 | 59.41 | 285.47 | 0.8574 | -260.0 | -278.4 | |
| 0.00 | 3.44 | 0.00 | 3.25 | 16.73 | 261.38 | 59.04 | 285.49 | 0.8542 | -664.0 | -523.5 | |
| 0.00 | 0.97 | 0.00 | 0.87 | 13.36 | 259.60 | 57.26 | 281.55 | 0.8375 | 398.0 | 367.8 | |
| 0.00 | 2.12 | 0.00 | 1.89 | 13.19 | 259.37 | 57.03 | 281.36 | 0.8353 | -234.0 | -83.9 | |
| 0.00 | 0.79 | 0.00 | 0.74 | 16.93 | 260.93 | 58.59 | 285.75 | 0.8504 | -632.0 | -542.9 | |
| 0.00 | 1.23 | 0.00 | 1.10 | 13.55 | 259.16 | 56.82 | 281.79 | 0.8334 | 515.0 | 471.7 | |
| 0.00 | 3.17 | 0.00 | 2.85 | 14.29 | 259.45 | 57.11 | 282.67 | 0.8362 | -146.0 | 69.1 | |
| 0.97 | 10.58 | 0.86 | 9.39 | 14.07 | 259.19 | 56.85 | 282.42 | 0.8337 | 581.3 | 289.4 | |
| 0.53 | -21.00 | 0.47 | -21.00 | 13.85 | 258.99 | 56.65 | 282.15 | 0.8318 | 631.3 | 999999 | |
| 2.64 | 363.29 | 2.36 | 315.75 | 14.56 | 259.21 | 56.87 | 283.00 | 0.8340 | 604.0 | 123.9 | |
| 5.82 | -23.00 | 5.18 | -23.00 | 15.00 | 259.11 | 56.77 | 283.54 | 0.8332 | 453.6 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.16 | 14.62 | 258.66 | 56.33 | 283.09 | 0.8289 | 447.0 | 362.9 | |
| 5.02 | 26.88 | 4.35 | 23.25 | 14.59 | 257.98 | 55.65 | 283.08 | 0.8224 | 842.5 | 451.5 | |
| 21.59 | -23.00 | 18.84 | -23.00 | 15.52 | 258.24 | 55.91 | 284.20 | 0.8252 | 712.7 | 999999 | |
| 0.00 | 1.59 | 0.00 | 1.40 | 16.87 | 258.72 | 56.38 | 285.80 | 0.8304 | -377.0 | -351.8 | |
| 9.87 | -23.00 | 8.54 | -23.00 | 15.99 | 257.88 | 55.54 | 284.79 | 0.8220 | 707.3 | 999999 | |
| 30.76 | -23.00 | 26.39 | -23.00 | 16.36 | 257.49 | 55.15 | 285.27 | 0.8184 | 906.7 | 999999 | |
| 6.79 | -23.00 | 5.84 | -23.00 | 17.51 | 257.55 | 55.21 | 286.66 | 0.8198 | 613.3 | 999999 | |
| 1.15 | -23.00 | 0.98 | -23.00 | 17.24 | 257.43 | 55.09 | 286.35 | 0.8184 | 646.0 | 999999 | |
| 2.47 | -23.00 | 2.11 | -23.00 | 17.60 | 257.26 | 54.92 | 286.80 | 0.8170 | 828.1 | 999999 | |
| 1.76 | -23.00 | 1.49 | -23.00 | 16.80 | 256.80 | 54.46 | 285.86 | 0.8120 | 831.7 | 999999 | |
| 2.03 | -23.00 | 1.71 | -23.00 | 17.15 | 256.73 | 54.39 | 286.29 | 0.8116 | 773.1 | 999999 | |
| 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. | |