| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.30 | 152.36 | 28.21 | 113.88 | 8.31 | 132.77 | -45.92 | 72.08 | 0.7485 | 320.9 | 99.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.82 | 6.40 | 142.68 | -36.00 | 70.16 | 0.6232 | -622.0 | -480.8 | |
| 0.00 | 1.98 | 0.00 | 1.26 | 7.29 | 142.31 | -36.37 | 69.05 | 0.6322 | -787.0 | -676.9 | |
| 0.00 | 0.69 | 0.00 | 0.46 | 13.50 | 141.38 | -37.30 | 60.91 | 0.6767 | -500.0 | -508.1 | |
| 0.00 | 2.15 | 0.00 | 1.39 | 7.20 | 141.46 | -37.23 | 69.65 | 0.6425 | -658.0 | -495.7 | |
| 0.00 | 1.12 | 0.00 | 0.72 | 7.43 | 141.28 | -37.40 | 69.41 | 0.6457 | -559.0 | -423.3 | |
| 0.00 | 1.72 | 0.00 | 1.13 | 7.99 | 140.73 | -37.95 | 68.89 | 0.6552 | -492.0 | -413.0 | |
| 0.00 | 0.95 | 0.00 | 0.62 | 7.30 | 140.57 | -38.11 | 69.97 | 0.6539 | -520.0 | -428.4 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 8.38 | 140.15 | -38.53 | 68.65 | 0.6640 | -517.0 | -392.4 | |
| 0.00 | 2.33 | 0.00 | 1.53 | 8.01 | 140.08 | -38.60 | 69.21 | 0.6632 | -714.0 | -609.9 | |
| 0.00 | 1.29 | 0.00 | 0.86 | 8.89 | 139.47 | -39.21 | 68.29 | 0.6746 | -612.0 | -534.5 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 5.30 | 139.33 | -39.35 | 73.46 | 0.6610 | -619.0 | -443.8 | |
| 0.95 | 2.67 | 0.67 | 1.90 | 7.40 | 135.04 | -43.64 | 72.40 | 0.7204 | -678.1 | -560.2 | |
| 0.43 | 2.33 | 0.32 | 1.71 | 6.80 | 132.92 | -45.77 | 74.02 | 0.7424 | -414.4 | -242.6 | |
| 0.00 | 0.95 | 0.00 | 0.70 | 6.90 | 132.86 | -45.82 | 73.92 | 0.7433 | 105.0 | 37.9 | |
| 7.15 | 128.16 | 5.38 | 97.39 | 8.81 | 132.37 | -46.31 | 71.66 | 0.7552 | 918.0 | 199.7 | |
| 0.00 | 1.12 | 0.00 | 0.83 | 7.17 | 132.57 | -46.11 | 73.68 | 0.7475 | 665.0 | 501.4 | |
| 28.77 | -15.00 | 21.84 | -15.00 | 8.34 | 131.79 | -46.90 | 72.47 | 0.7599 | 708.3 | 999999 | |
| 0.00 | 1.55 | 0.00 | 1.20 | 8.42 | 130.66 | -48.02 | 72.80 | 0.7721 | 291.0 | 213.7 | |
| 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. | |