| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.88 | 42.03 | 11.86 | 33.96 | -17.45 | 206.15 | -46.58 | 118.70 | 0.7916 | 225.6 | 121.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.15 | 16.76 | 1.68 | 13.11 | -17.70 | 208.13 | -44.61 | 119.97 | 0.7746 | 734.5 | 476.4 | |
| 8.15 | -1.00 | 6.39 | -1.00 | -17.56 | 207.81 | -44.92 | 119.65 | 0.7769 | 624.5 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.78 | -17.89 | 207.48 | -45.26 | 119.86 | 0.7816 | -81.0 | -27.0 | |
| 0.81 | 2.06 | 0.61 | 1.57 | -15.00 | 208.30 | -44.44 | 116.85 | 0.7603 | 645.7 | 519.9 | |
| 0.00 | 1.61 | 0.00 | 1.28 | -17.31 | 206.99 | -45.75 | 118.93 | 0.7836 | 429.0 | 347.6 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -17.17 | 207.03 | -45.70 | 118.79 | 0.7825 | 485.0 | 444.0 | |
| 0.00 | 2.60 | 0.00 | 2.07 | -16.76 | 206.53 | -46.21 | 118.05 | 0.7855 | 647.0 | 482.5 | |
| 0.72 | 1.88 | 0.59 | 1.55 | -18.74 | 205.80 | -46.94 | 119.98 | 0.8010 | 330.5 | 296.5 | |
| 0.00 | 1.52 | 0.00 | 1.21 | -16.41 | 206.45 | -46.28 | 117.61 | 0.7847 | 701.0 | 601.0 | |
| 0.54 | 2.96 | 0.43 | 2.36 | -16.58 | 206.31 | -46.43 | 117.74 | 0.7868 | 458.3 | 352.6 | |
| 1.16 | 5.02 | 0.99 | 4.24 | -18.55 | 204.35 | -48.39 | 119.06 | 0.8131 | -665.6 | -451.3 | |
| 0.90 | -11.00 | 0.76 | -11.00 | -18.38 | 204.36 | -48.38 | 118.87 | 0.8123 | -440.7 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.72 | -19.70 | 202.49 | -50.24 | 119.48 | 0.8336 | -492.0 | -475.3 | |
| 0.00 | 2.06 | 0.00 | 1.74 | -16.19 | 203.55 | -49.18 | 116.01 | 0.8109 | -572.0 | -487.4 | |
| 0.00 | 0.54 | 0.00 | 0.47 | -17.78 | 202.43 | -50.31 | 117.32 | 0.8268 | -444.0 | -505.7 | |
| 0.00 | 1.61 | 0.00 | 1.42 | -17.67 | 202.22 | -50.51 | 117.10 | 0.8282 | -516.0 | -430.0 | |
| 0.45 | 1.34 | 0.41 | 1.23 | -17.75 | 200.40 | -52.34 | 116.43 | 0.8441 | -336.8 | -323.7 | |
| 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. | |