SOHO MDI 2000-07-15 11:13:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 388 | 36 | 210 | 2.90 | 270.67 | -24.08 | 92.98 | 0.4094 | -810.8 | -280.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 4 | -0.59 | 278.47 | -16.27 | 106.84 | 0.2941 | 238.0 | 110.9 | |
| 0 | 5 | 0 | 2 | 1.33 | 277.35 | -17.39 | 99.68 | 0.3045 | 525.0 | 439.3 | |
| 10 | 25 | 5 | 13 | 2.66 | 276.96 | -17.78 | 95.16 | 0.3077 | 1276.6 | 781.5 | |
| 0 | 30 | 0 | 16 | 3.79 | 275.94 | -18.80 | 91.34 | 0.3231 | 737.0 | 602.4 | |
| 4 | 28 | 2 | 15 | 3.00 | 274.70 | -20.05 | 93.45 | 0.3445 | 851.9 | 893.4 | |
| 0 | 10 | 0 | 5 | 3.07 | 272.96 | -21.79 | 92.87 | 0.3727 | 305.0 | 292.3 | |
| 0 | 8 | 0 | 4 | 3.90 | 271.39 | -23.36 | 90.49 | 0.3972 | -963.0 | -835.6 | |
| 0 | 3 | 0 | 2 | 2.70 | 269.99 | -24.76 | 93.20 | 0.4208 | -749.0 | -552.7 | |
| 17 | 215 | 9 | 118 | 3.50 | 269.00 | -25.74 | 91.18 | 0.4354 | -1499.3 | -648.6 | |
| 0 | 6 | 0 | 3 | 1.33 | 269.05 | -25.70 | 96.17 | 0.4379 | -474.0 | -450.0 | |
| 9 | -9 | 5 | -9 | 2.99 | 268.97 | -25.77 | 92.36 | 0.4364 | -1698.2 | 999999 | |
| 8 | -9 | 5 | -9 | 3.13 | 268.57 | -26.17 | 91.97 | 0.4425 | -1229.9 | 999999 | |
| 13 | 51 | 7 | 28 | 1.86 | 268.51 | -26.24 | 94.81 | 0.4452 | -1095.9 | -450.7 | |
| 6 | -9 | 3 | -9 | 2.61 | 268.36 | -26.38 | 93.11 | 0.4464 | -842.7 | 999999 | |
| 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. | |