SOHO MDI 2000-10-29 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37 | 496 | 36 | 490 | 9.31 | 268.11 | -60.28 | 81.84 | 0.8677 | 653.5 | 124.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 5 | 8.38 | 271.63 | -56.76 | 82.92 | 0.8360 | 150.0 | 182.5 | |
| 0 | 4 | 0 | 4 | 10.39 | 270.68 | -57.71 | 80.55 | 0.8451 | 496.0 | 449.4 | |
| 0 | 5 | 0 | 5 | 9.77 | 270.26 | -58.13 | 81.28 | 0.8489 | 469.0 | 480.9 | |
| 0 | 4 | 0 | 4 | 9.27 | 270.32 | -58.07 | 81.87 | 0.8482 | 528.0 | 462.7 | |
| 0 | 5 | 0 | 5 | 9.00 | 269.79 | -58.60 | 82.19 | 0.8530 | 417.0 | 362.2 | |
| 0 | 6 | 0 | 5 | 6.43 | 269.76 | -58.63 | 85.21 | 0.8535 | 123.0 | 162.5 | |
| 5 | 418 | 5 | 413 | 8.78 | 268.86 | -59.54 | 82.45 | 0.8614 | 504.1 | 162.4 | |
| 17 | -7 | 16 | -7 | 9.73 | 268.51 | -59.88 | 81.35 | 0.8644 | 1239.4 | 999999 | |
| 0 | 13 | 0 | 12 | 6.88 | 268.92 | -59.48 | 84.66 | 0.8610 | -328.0 | -300.0 | |
| 5 | -7 | 5 | -7 | 10.00 | 267.87 | -60.52 | 81.04 | 0.8699 | 885.9 | 999999 | |
| 4 | -7 | 4 | -7 | 9.68 | 267.65 | -60.74 | 81.42 | 0.8718 | 570.8 | 999999 | |
| 0 | 5 | 0 | 5 | 6.90 | 268.05 | -60.34 | 84.62 | 0.8685 | -210.0 | -258.5 | |
| 6 | -7 | 6 | -7 | 8.91 | 267.23 | -61.16 | 82.30 | 0.8753 | -563.5 | 999999 | |
| 0 | 6 | 0 | 6 | 6.61 | 267.15 | -61.24 | 84.93 | 0.8762 | -365.0 | -473.4 | |
| 0 | 3 | 0 | 3 | 12.05 | 264.56 | -63.83 | 78.77 | 0.8967 | -344.0 | -326.9 | |
| 0 | 6 | 0 | 7 | 9.46 | 265.03 | -63.36 | 81.67 | 0.8930 | -289.0 | -190.7 | |
| 0 | 2 | 0 | 2 | 11.59 | 264.22 | -64.18 | 79.29 | 0.8993 | -371.0 | -318.2 | |
| 0 | 5 | 0 | 6 | 11.29 | 263.88 | -64.51 | 79.62 | 0.9017 | -602.0 | -487.6 | |
| 0 | 6 | 0 | 6 | 3.65 | 265.83 | -62.56 | 88.23 | 0.8881 | -369.0 | -240.3 | |
| 0 | 2 | 0 | 2 | 10.51 | 263.83 | -64.56 | 80.50 | 0.9021 | -278.0 | -320.0 | |
| 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. | |