SOHO MDI 2000-07-13 17:00:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88 | 504 | 159 | 1068 | -18.32 | 32.15 | 74.12 | 249.87 | 0.9686 | 374.0 | 1.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2 | 96 | 8 | 390 | -17.35 | 37.73 | 79.70 | 251.73 | 0.9897 | 37.9 | 27.1 | |
| 6 | -1 | 25 | -1 | -18.54 | 39.62 | 81.58 | 250.75 | 0.9939 | 266.5 | 999999 | |
| 0 | 4 | 0 | 10 | -16.58 | 35.28 | 77.24 | 252.19 | 0.9827 | -195.0 | -179.3 | |
| 0 | 7 | 0 | 20 | -18.10 | 36.52 | 78.49 | 250.82 | 0.9869 | -411.0 | -272.9 | |
| 0 | 2 | 0 | 5 | -17.62 | 34.63 | 76.59 | 251.05 | 0.9811 | -151.0 | -99.8 | |
| 0 | 11 | 0 | 23 | -16.82 | 32.95 | 74.91 | 251.61 | 0.9749 | -463.0 | -394.5 | |
| 0 | 2 | 0 | 5 | -17.94 | 32.18 | 74.14 | 250.36 | 0.9728 | -392.0 | -380.6 | |
| 0 | 5 | 0 | 9 | -17.01 | 29.24 | 71.20 | 250.83 | 0.9597 | -383.0 | -461.2 | |
| 0 | 7 | 0 | 11 | -16.50 | 26.73 | 68.69 | 250.91 | 0.9467 | 148.0 | 72.6 | |
| 12 | 202 | 20 | 351 | -18.69 | 28.50 | 70.46 | 248.97 | 0.9577 | 197.5 | -182.0 | |
| 13 | 63 | 20 | 92 | -15.77 | 25.97 | 67.93 | 251.52 | 0.9418 | 721.4 | 291.2 | |
| 26 | -10 | 45 | -10 | -19.74 | 28.92 | 70.88 | 247.97 | 0.9606 | 218.3 | 999999 | |
| 6 | 34 | 8 | 48 | -16.96 | 24.96 | 66.93 | 250.08 | 0.9375 | 720.1 | 435.2 | |
| 15 | 71 | 21 | 104 | -18.42 | 25.32 | 67.29 | 248.63 | 0.9413 | 627.0 | 283.1 | |
| 8 | -14 | 12 | -14 | -18.99 | 25.57 | 67.54 | 248.09 | 0.9433 | 522.3 | 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. | |