SOHO MDI 2000-10-26 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81 | 388 | 95 | 460 | -22.88 | 307.41 | -60.52 | 117.95 | 0.9092 | -444.9 | -65.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 40 | 17 | 44 | -23.98 | 309.96 | -57.97 | 119.90 | 0.8954 | -592.2 | -393.1 | |
| 11 | 86 | 13 | 100 | -23.83 | 308.43 | -59.50 | 119.25 | 0.9052 | -644.7 | -59.7 | |
| 4 | -2 | 5 | -2 | -23.47 | 308.11 | -59.81 | 118.77 | 0.9064 | -381.4 | 999999 | |
| 18 | 116 | 20 | 131 | -22.18 | 308.62 | -59.30 | 117.57 | 0.9001 | -709.3 | -137.3 | |
| 0 | 13 | 0 | 14 | -20.45 | 309.75 | -58.18 | 116.07 | 0.8882 | 627.0 | 530.8 | |
| 7 | -2 | 8 | -2 | -23.56 | 307.44 | -60.48 | 118.66 | 0.9109 | -77.1 | 999999 | |
| 5 | 16 | 5 | 18 | -20.40 | 308.08 | -59.84 | 115.51 | 0.8998 | 727.7 | 559.0 | |
| 1 | 9 | 1 | 11 | -22.33 | 306.74 | -61.19 | 117.16 | 0.9127 | -219.0 | -136.0 | |
| 0 | 3 | 0 | 4 | -21.63 | 307.00 | -60.93 | 116.50 | 0.9096 | 297.0 | 279.0 | |
| 19 | 83 | 26 | 110 | -23.95 | 304.69 | -63.24 | 118.27 | 0.9282 | -434.8 | -78.3 | |
| 0 | 2 | 0 | 3 | -19.94 | 307.55 | -60.37 | 114.86 | 0.9025 | 335.0 | 346.2 | |
| -10 | -10 | -10 | -10 | -23.58 | 304.45 | -63.48 | 117.82 | 0.9289 | 999999 | 999999 | |
| 0 | 11 | 0 | 13 | -20.93 | 306.19 | -61.73 | 115.53 | 0.9134 | 598.0 | 505.0 | |
| 0 | 2 | 0 | 2 | -22.52 | 304.78 | -63.14 | 116.82 | 0.9251 | -297.0 | -248.0 | |
| 0 | 7 | 0 | 10 | -21.82 | 303.36 | -64.56 | 115.72 | 0.9321 | -344.0 | -427.2 | |
| 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. | |