| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.81 | 302.19 | 33.10 | 167.54 | -23.81 | 192.76 | -16.72 | 144.16 | 0.4510 | 736.0 | 383.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.40 | 277.12 | 10.71 | 153.36 | -23.65 | 193.43 | -16.06 | 144.93 | 0.4429 | 1332.3 | 416.8 | |
| 1.44 | -1.00 | 0.80 | -1.00 | -24.01 | 193.38 | -16.11 | 145.36 | 0.4477 | 672.1 | 999999 | |
| 8.71 | -1.00 | 4.82 | -1.00 | -23.58 | 193.02 | -16.46 | 144.18 | 0.4457 | 1224.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -22.70 | 192.96 | -16.52 | 142.79 | 0.4357 | 802.0 | 586.7 | |
| 26.40 | -1.00 | 14.65 | -1.00 | -23.96 | 192.76 | -16.72 | 144.32 | 0.4527 | 1020.6 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -23.24 | 191.93 | -17.56 | 141.98 | 0.4520 | 622.0 | 528.5 | |
| 3.05 | 4.49 | 1.67 | 2.46 | -21.53 | 192.08 | -17.40 | 139.57 | 0.4308 | -947.2 | -703.0 | |
| 0.81 | 6.91 | 0.45 | 3.85 | -23.13 | 191.46 | -18.03 | 141.12 | 0.4553 | 1115.6 | 716.7 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -23.72 | 191.37 | -18.11 | 141.86 | 0.4628 | 555.0 | 446.0 | |
| 0.00 | 2.33 | 0.00 | 1.30 | -22.84 | 191.15 | -18.33 | 140.22 | 0.4550 | 551.0 | 561.8 | |
| 0.00 | 1.62 | 0.00 | 0.93 | -25.26 | 187.42 | -22.06 | 138.83 | 0.5181 | -814.0 | -661.6 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -25.98 | 186.84 | -22.64 | 139.14 | 0.5311 | -752.0 | -616.5 | |
| 0.00 | 1.80 | 0.00 | 1.06 | -27.00 | 186.33 | -23.16 | 139.93 | 0.5464 | -811.0 | -682.4 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -26.38 | 185.43 | -24.06 | 138.10 | 0.5489 | -630.0 | -550.3 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -24.99 | 185.44 | -24.05 | 136.17 | 0.5354 | -614.0 | -588.7 | |
| 0.00 | 0.72 | 0.00 | 0.44 | -28.36 | 183.63 | -25.86 | 138.82 | 0.5851 | -691.0 | -629.6 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -28.05 | 183.60 | -25.89 | 138.40 | 0.5826 | -720.0 | -621.0 | |
| 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. | |