| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.74 | 219.15 | 49.05 | 200.64 | -19.64 | 107.24 | -51.38 | 118.97 | 0.8432 | 646.1 | 277.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.41 | -23.05 | 109.13 | -49.49 | 123.54 | 0.8414 | -409.0 | -349.0 | |
| 0.00 | 0.80 | 0.00 | 0.75 | -22.58 | 107.72 | -50.90 | 122.37 | 0.8505 | 267.0 | 291.2 | |
| 1.07 | 4.46 | 1.00 | 4.19 | -22.36 | 107.52 | -51.10 | 122.04 | 0.8512 | 620.3 | 505.5 | |
| 0.00 | 1.34 | 0.00 | 1.20 | -19.75 | 108.19 | -50.42 | 119.52 | 0.8358 | 700.0 | 563.1 | |
| 0.00 | 0.80 | 0.00 | 0.76 | -22.04 | 107.00 | -51.62 | 121.47 | 0.8539 | 359.0 | 355.1 | |
| 0.00 | 1.61 | 0.00 | 1.45 | -19.62 | 107.85 | -50.77 | 119.22 | 0.8382 | 579.0 | 433.6 | |
| 20.89 | 76.32 | 18.61 | 67.73 | -18.68 | 108.00 | -50.62 | 118.24 | 0.8334 | 852.6 | 472.6 | |
| 8.57 | 119.53 | 7.95 | 111.04 | -20.57 | 107.16 | -51.46 | 119.95 | 0.8473 | 651.3 | 174.6 | |
| 0.00 | 1.25 | 0.00 | 1.14 | -19.34 | 107.36 | -51.26 | 118.70 | 0.8412 | 654.0 | 541.8 | |
| 8.66 | -8.00 | 8.04 | -8.00 | -20.12 | 106.90 | -51.72 | 119.35 | 0.8478 | 772.2 | 999999 | |
| 8.66 | -8.00 | 8.02 | -8.00 | -19.83 | 106.82 | -51.79 | 119.00 | 0.8473 | 759.1 | 999999 | |
| 4.91 | 7.41 | 4.51 | 6.80 | -19.12 | 106.88 | -51.73 | 118.25 | 0.8443 | 638.4 | 442.1 | |
| 0.98 | -8.00 | 0.92 | -8.00 | -19.87 | 106.38 | -52.24 | 118.86 | 0.8510 | -79.9 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.97 | -19.72 | 104.41 | -54.21 | 117.88 | 0.8659 | 569.0 | 492.7 | |
| 0.00 | 1.70 | 0.00 | 1.68 | -18.31 | 103.60 | -55.02 | 116.05 | 0.8678 | -333.0 | -247.0 | |
| 0.00 | 0.98 | 0.00 | 0.99 | -18.33 | 103.08 | -55.54 | 115.88 | 0.8719 | -290.0 | -278.2 | |
| 0.00 | 1.52 | 0.00 | 1.53 | -17.96 | 102.87 | -55.75 | 115.40 | 0.8724 | -709.0 | -580.4 | |
| 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. | |