SOHO MDI 2000-09-22 04:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68 | 293 | 37 | 166 | -5.49 | 80.87 | -25.08 | 116.16 | 0.4716 | -472.1 | -32.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23 | 69 | 12 | 38 | -5.91 | 84.22 | -21.73 | 120.31 | 0.4285 | -1432.1 | -851.1 | |
| 3 | -1 | 2 | -1 | -5.36 | 83.99 | -21.96 | 118.93 | 0.4273 | -978.8 | 999999 | |
| 13 | 54 | 7 | 30 | -6.01 | 82.95 | -23.01 | 119.06 | 0.4466 | -1190.9 | -625.2 | |
| 7 | -3 | 4 | -3 | -6.11 | 82.64 | -23.31 | 118.92 | 0.4515 | -987.2 | 999999 | |
| 0 | 7 | 0 | 4 | -6.61 | 82.10 | -23.85 | 119.32 | 0.4626 | -792.0 | -549.5 | |
| 0 | 4 | 0 | 2 | -4.94 | 81.96 | -23.99 | 115.93 | 0.4523 | -501.0 | -459.9 | |
| 0 | 7 | 0 | 4 | -3.76 | 80.93 | -25.03 | 112.62 | 0.4592 | 990.0 | 734.3 | |
| 0 | 6 | 0 | 3 | -6.29 | 80.65 | -25.31 | 117.24 | 0.4799 | 665.0 | 516.7 | |
| 0 | 4 | 0 | 3 | -7.21 | 80.60 | -25.36 | 118.89 | 0.4873 | 723.0 | 565.6 | |
| 0 | 7 | 0 | 4 | -4.06 | 80.57 | -25.38 | 112.90 | 0.4661 | 675.0 | 474.5 | |
| 0 | 5 | 0 | 3 | -4.72 | 79.42 | -26.54 | 113.20 | 0.4865 | 441.0 | 481.7 | |
| 4 | 130 | 2 | 75 | -4.79 | 78.84 | -27.11 | 112.87 | 0.4949 | 1084.5 | 524.6 | |
| 10 | -12 | 5 | -12 | -5.09 | 78.48 | -27.48 | 113.13 | 0.5018 | 1226.8 | 999999 | |
| 5 | -12 | 3 | -12 | -5.51 | 78.23 | -27.72 | 113.69 | 0.5077 | 865.5 | 999999 | |
| 3 | -12 | 2 | -12 | -5.16 | 78.07 | -27.88 | 112.93 | 0.5077 | 980.4 | 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. | |