SOHO MDI 2000-10-30 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20 | 145 | 14 | 96 | -28.07 | 292.96 | -24.89 | 145.04 | 0.6502 | 883.3 | 614.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -26.54 | 297.28 | -20.57 | 148.36 | 0.6015 | 709.0 | 612.9 | |
| 0 | 4 | 0 | 3 | -29.05 | 295.63 | -22.22 | 148.83 | 0.6410 | 776.0 | 693.2 | |
| 0 | 4 | 0 | 2 | -28.37 | 295.45 | -22.39 | 148.00 | 0.6349 | 773.0 | 662.5 | |
| 4 | 16 | 3 | 10 | -26.70 | 295.21 | -22.64 | 146.08 | 0.6187 | 1051.4 | 760.0 | |
| 0 | 6 | 0 | 4 | -27.56 | 294.92 | -22.93 | 146.63 | 0.6301 | 765.0 | 681.6 | |
| 0 | 11 | 0 | 7 | -26.29 | 293.88 | -23.96 | 144.19 | 0.6247 | 940.0 | 834.2 | |
| 6 | 50 | 4 | 33 | -29.52 | 292.67 | -25.18 | 146.15 | 0.6670 | 961.9 | 518.6 | |
| 7 | -7 | 5 | -7 | -29.30 | 292.43 | -25.42 | 145.69 | 0.6665 | 894.7 | 999999 | |
| 0 | 6 | 0 | 4 | -27.91 | 292.74 | -25.11 | 144.64 | 0.6502 | 763.0 | 560.1 | |
| 3 | 7 | 2 | 5 | -28.80 | 292.08 | -25.77 | 144.85 | 0.6642 | 711.1 | 602.3 | |
| 0 | 17 | 0 | 11 | -26.84 | 292.19 | -25.66 | 142.97 | 0.6439 | 862.0 | 788.0 | |
| 0 | 5 | 0 | 3 | -26.35 | 292.26 | -25.59 | 142.52 | 0.6384 | 728.0 | 649.0 | |
| 0 | 2 | 0 | 2 | -28.96 | 291.54 | -26.31 | 144.48 | 0.6698 | 569.0 | 471.5 | |
| 0 | 4 | 0 | 3 | -29.44 | 290.91 | -26.94 | 144.35 | 0.6792 | 123.0 | 290.8 | |
| 0 | 4 | 0 | 3 | -27.34 | 291.00 | -26.85 | 142.29 | 0.6583 | 360.0 | 375.5 | |
| 0 | 6 | 0 | 4 | -27.04 | 289.47 | -28.38 | 140.50 | 0.6680 | 578.0 | 565.5 | |
| 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. | |