SOHO MDI 2000-07-18 03:14:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62 | 519 | 36 | 306 | 19.03 | 289.21 | 29.78 | 298.88 | 0.5377 | 345.3 | 177.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 5 | 21.71 | 292.12 | 32.69 | 301.26 | 0.5892 | 703.0 | 606.3 | |
| 14 | 301 | 8 | 180 | 19.32 | 291.16 | 31.72 | 298.00 | 0.5642 | 1307.3 | 683.0 | |
| 17 | -2 | 10 | -2 | 18.46 | 290.97 | 31.54 | 296.68 | 0.5575 | 1658.2 | 999999 | |
| 7 | -2 | 4 | -2 | 18.84 | 290.86 | 31.42 | 297.38 | 0.5578 | 1560.3 | 999999 | |
| 0 | 5 | 0 | 3 | 18.36 | 289.40 | 29.97 | 297.48 | 0.5365 | 511.0 | 408.2 | |
| 0 | 8 | 0 | 4 | 19.15 | 289.26 | 29.83 | 298.92 | 0.5390 | 611.0 | 473.9 | |
| 0 | 7 | 0 | 4 | 18.56 | 288.57 | 29.14 | 298.37 | 0.5267 | -164.0 | -39.0 | |
| 3 | 9 | 2 | 5 | 18.90 | 288.30 | 28.87 | 299.16 | 0.5252 | -309.6 | -218.6 | |
| 0 | 4 | 0 | 2 | 20.35 | 288.01 | 28.58 | 301.88 | 0.5303 | 306.0 | 335.2 | |
| 0 | 4 | 0 | 3 | 18.50 | 286.95 | 27.52 | 299.43 | 0.5051 | -513.0 | -465.9 | |
| 0 | 4 | 0 | 3 | 20.84 | 287.05 | 27.62 | 303.48 | 0.5216 | -502.0 | -372.3 | |
| 0 | 6 | 0 | 3 | 21.05 | 286.81 | 27.38 | 304.05 | 0.5201 | -896.0 | -694.6 | |
| 21 | 147 | 12 | 84 | 18.94 | 285.95 | 26.52 | 301.04 | 0.4948 | -1598.9 | -762.9 | |
| 0 | 8 | 0 | 5 | 21.11 | 286.25 | 26.82 | 304.63 | 0.5136 | -728.0 | -632.8 | |
| 0 | 5 | 0 | 3 | 20.82 | 285.25 | 25.82 | 305.01 | 0.4990 | -426.0 | -501.2 | |
| 0 | 3 | 0 | 2 | 21.14 | 284.28 | 24.84 | 306.50 | 0.4895 | -335.0 | -421.6 | |
| 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. | |