SOHO MDI 2002-08-02 06:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 394 | 34 | 202 | -8.29 | 144.92 | 1.05 | 184.42 | 0.2517 | 92.3 | 233.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 146 | 4 | 74 | -7.88 | 148.74 | 4.87 | 199.50 | 0.2531 | -799.0 | -155.3 | |
| 5 | -1 | 2 | -1 | -7.11 | 148.69 | 4.82 | 200.39 | 0.2405 | 1170.8 | 999999 | |
| 15 | -1 | 8 | -1 | -7.92 | 148.14 | 4.27 | 197.20 | 0.2505 | -1605.7 | 999999 | |
| 0 | 5 | 0 | 2 | -6.86 | 147.81 | 3.94 | 197.21 | 0.2316 | 341.0 | 205.7 | |
| 0 | 6 | 0 | 3 | -8.11 | 147.30 | 3.43 | 193.78 | 0.2499 | -903.0 | -723.9 | |
| 0 | 4 | 0 | 2 | -7.70 | 146.82 | 2.95 | 192.25 | 0.2413 | -852.0 | -632.8 | |
| 9 | 30 | 5 | 15 | -8.15 | 145.50 | 1.63 | 186.64 | 0.2451 | -1279.3 | -704.4 | |
| 0 | 7 | 0 | 4 | -8.47 | 144.34 | 0.47 | 181.89 | 0.2491 | 629.0 | 663.2 | |
| 0 | 7 | 0 | 4 | -7.94 | 143.74 | -0.12 | 179.48 | 0.2400 | 667.0 | 541.6 | |
| 0 | 5 | 0 | 2 | -7.37 | 143.70 | -0.16 | 179.29 | 0.2303 | 737.0 | 542.8 | |
| 0 | 3 | 0 | 2 | -9.82 | 143.46 | -0.41 | 178.52 | 0.2720 | -809.0 | -588.8 | |
| 3 | 13 | 1 | 7 | -8.18 | 143.34 | -0.52 | 177.87 | 0.2443 | 1096.6 | 870.6 | |
| 0 | 15 | 0 | 8 | -7.74 | 142.75 | -1.12 | 175.29 | 0.2373 | 905.0 | 804.0 | |
| 20 | 119 | 10 | 61 | -9.04 | 141.94 | -1.93 | 172.65 | 0.2608 | 1737.6 | 684.1 | |
| 0 | 9 | 0 | 5 | -8.35 | 141.90 | -1.96 | 172.15 | 0.2492 | 848.0 | 833.0 | |
| 8 | 25 | 4 | 13 | -8.39 | 141.50 | -2.36 | 170.60 | 0.2510 | 1154.3 | 692.6 | |
| 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. | |