SOHO MDI 2000-07-17 09:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70 | 547 | 38 | 299 | 19.21 | 289.16 | 19.99 | 308.57 | 0.4143 | 312.0 | 229.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21 | 327 | 12 | 179 | 19.49 | 290.67 | 21.51 | 307.14 | 0.4353 | 1521.0 | 725.6 | |
| 0 | 8 | 0 | 5 | 23.16 | 291.16 | 21.99 | 313.19 | 0.4741 | 771.0 | 698.1 | |
| 13 | -1 | 7 | -1 | 18.40 | 290.35 | 21.18 | 305.34 | 0.4220 | 1846.6 | 999999 | |
| 8 | -1 | 4 | -1 | 18.77 | 290.35 | 21.18 | 306.08 | 0.4251 | 1823.3 | 999999 | |
| 0 | 5 | 0 | 3 | 19.61 | 289.30 | 20.13 | 309.06 | 0.4193 | 325.0 | 301.5 | |
| 0 | 4 | 0 | 2 | 18.56 | 288.94 | 19.78 | 307.39 | 0.4054 | 339.0 | 303.2 | |
| 0 | 11 | 0 | 6 | 19.75 | 288.69 | 19.52 | 310.13 | 0.4131 | -505.0 | -428.4 | |
| 0 | 6 | 0 | 3 | 20.25 | 288.58 | 19.41 | 311.25 | 0.4164 | 738.0 | 588.0 | |
| 0 | 3 | 0 | 2 | 19.23 | 288.23 | 19.06 | 309.72 | 0.4026 | -241.0 | -253.9 | |
| 0 | 5 | 0 | 3 | 20.59 | 288.22 | 19.05 | 312.39 | 0.4155 | 362.0 | 345.9 | |
| 28 | 152 | 15 | 82 | 18.94 | 286.74 | 17.57 | 311.28 | 0.3816 | -1708.7 | -709.5 | |
| 0 | 5 | 0 | 2 | 21.16 | 286.55 | 17.38 | 315.94 | 0.4024 | -863.0 | -757.3 | |
| 0 | 5 | 0 | 3 | 20.67 | 286.49 | 17.33 | 315.10 | 0.3964 | -896.0 | -661.4 | |
| 0 | 7 | 0 | 4 | 21.55 | 285.80 | 16.63 | 317.85 | 0.3984 | -928.0 | -720.0 | |
| 0 | 5 | 0 | 3 | 21.81 | 285.47 | 16.31 | 318.85 | 0.3978 | -752.0 | -644.8 | |
| 0 | 4 | 0 | 2 | 18.81 | 285.11 | 15.94 | 313.63 | 0.3608 | 470.0 | 317.4 | |
| 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. | |