SOHO MDI 2000-07-13 07:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 77 | 2 | 41 | -14.96 | 321.38 | -1.63 | 175.74 | 0.3335 | 645.1 | 71.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 14 | 0 | 7 | -12.76 | 325.16 | 2.16 | 187.15 | 0.2960 | -948.0 | -719.5 | |
| 0 | 3 | 0 | 2 | -12.43 | 324.63 | 1.63 | 185.52 | 0.2895 | -1018.0 | -895.2 | |
| 0 | 9 | 0 | 5 | -12.26 | 324.27 | 1.26 | 184.32 | 0.2862 | -1320.0 | -1078.7 | |
| 0 | 5 | 0 | 3 | -11.97 | 323.66 | 0.65 | 182.28 | 0.2808 | -930.0 | -676.0 | |
| 0 | 4 | 0 | 2 | -11.73 | 321.03 | -1.98 | 173.00 | 0.2784 | 781.0 | 730.5 | |
| 0 | 4 | 0 | 2 | -21.84 | 320.92 | -2.09 | 175.60 | 0.4429 | 638.0 | 595.6 | |
| 0 | 4 | 0 | 2 | -26.35 | 319.74 | -3.27 | 174.27 | 0.5135 | 701.0 | 544.0 | |
| 0 | 5 | 0 | 3 | -26.54 | 319.02 | -3.98 | 173.08 | 0.5175 | 654.0 | 625.8 | |
| 3 | 8 | 2 | 4 | -14.14 | 319.13 | -3.88 | 168.25 | 0.3234 | 1190.7 | 829.5 | |
| 0 | 5 | 0 | 3 | -14.23 | 318.56 | -4.45 | 166.63 | 0.3269 | 946.0 | 783.6 | |
| 0 | 6 | 0 | 3 | -11.20 | 318.57 | -4.44 | 164.08 | 0.2780 | 641.0 | 621.3 | |
| 0 | 3 | 0 | 2 | -13.77 | 318.44 | -4.57 | 165.95 | 0.3200 | 904.0 | 841.4 | |
| 0 | 4 | 0 | 2 | -13.98 | 318.07 | -4.94 | 165.03 | 0.3249 | 983.0 | 760.9 | |
| 0 | 3 | 0 | 1 | -14.03 | 317.54 | -5.47 | 163.54 | 0.3280 | 899.0 | 807.5 | |
| 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. | |