SOHO MDI 2000-11-05 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56 | 405 | 34 | 241 | 2.55 | 271.92 | 34.01 | 268.95 | 0.5604 | 1369.6 | 592.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17 | 349 | 11 | 211 | 2.28 | 273.53 | 35.62 | 268.62 | 0.5844 | 1269.3 | 702.8 | |
| 10 | -1 | 6 | -1 | 2.10 | 273.15 | 35.24 | 268.27 | 0.5791 | 1488.9 | 999999 | |
| 0 | 3 | 0 | 2 | 3.92 | 272.93 | 35.02 | 271.42 | 0.5749 | 373.0 | 354.1 | |
| 4 | -1 | 2 | -1 | 3.23 | 272.76 | 34.85 | 270.21 | 0.5727 | 1035.2 | 999999 | |
| 7 | -1 | 4 | -1 | 2.97 | 272.47 | 34.56 | 269.74 | 0.5687 | 1508.9 | 999999 | |
| 18 | -1 | 11 | -1 | 2.63 | 272.36 | 34.45 | 269.12 | 0.5674 | 1718.4 | 999999 | |
| 0 | 6 | 0 | 3 | 3.54 | 271.70 | 33.79 | 270.70 | 0.5573 | 927.0 | 763.3 | |
| 0 | 4 | 0 | 2 | -0.22 | 271.35 | 33.44 | 263.89 | 0.5563 | 638.0 | 533.9 | |
| 0 | 4 | 0 | 2 | 2.28 | 269.32 | 31.41 | 268.16 | 0.5231 | 516.0 | 477.5 | |
| 0 | 5 | 0 | 3 | 3.81 | 266.12 | 28.21 | 270.99 | 0.4737 | 687.0 | 571.2 | |
| 0 | 8 | 0 | 4 | 2.97 | 263.20 | 25.29 | 268.93 | 0.4285 | -851.0 | -744.4 | |
| 0 | 6 | 0 | 3 | 2.05 | 263.10 | 25.19 | 266.76 | 0.4278 | -865.0 | -691.0 | |
| 0 | 4 | 0 | 2 | 3.78 | 262.97 | 25.06 | 270.83 | 0.4245 | -680.0 | -536.0 | |
| 0 | 7 | 0 | 4 | 2.95 | 260.92 | 23.01 | 268.63 | 0.3922 | -983.0 | -792.7 | |
| 0 | 5 | 0 | 3 | 2.57 | 260.78 | 22.88 | 267.63 | 0.3904 | -723.0 | -635.0 | |
| 0 | 4 | 0 | 2 | 4.09 | 256.82 | 18.91 | 271.56 | 0.3248 | -664.0 | -480.2 | |
| 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. | |