SOHO MDI 2000-11-06 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66 | 529 | 40 | 318 | 19.12 | 254.92 | 31.94 | 299.24 | 0.5735 | 1216.8 | 359.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52 | 410 | 32 | 252 | 19.12 | 256.77 | 33.80 | 297.77 | 0.5962 | 1494.9 | 615.8 | |
| 0 | 7 | 0 | 4 | 17.67 | 255.97 | 32.99 | 295.89 | 0.5790 | 529.0 | 606.1 | |
| 9 | -1 | 5 | -1 | 18.91 | 256.04 | 33.06 | 297.85 | 0.5860 | 1943.6 | 999999 | |
| 0 | 8 | 0 | 4 | 14.77 | 254.02 | 31.04 | 292.00 | 0.5399 | -128.0 | -326.8 | |
| 0 | 4 | 0 | 2 | 14.50 | 253.79 | 30.81 | 291.64 | 0.5357 | -505.0 | -446.0 | |
| 5 | 12 | 3 | 7 | 17.20 | 253.31 | 30.34 | 296.68 | 0.5422 | -924.1 | -753.9 | |
| 0 | 6 | 0 | 4 | 17.53 | 252.91 | 29.93 | 297.51 | 0.5386 | -910.0 | -698.0 | |
| 0 | 3 | 0 | 2 | 17.72 | 252.06 | 29.08 | 298.41 | 0.5286 | 287.0 | 323.9 | |
| 0 | 3 | 0 | 2 | 21.14 | 247.23 | 24.25 | 308.57 | 0.4920 | -327.0 | -342.7 | |
| 0 | 4 | 0 | 2 | 20.62 | 246.87 | 23.89 | 308.06 | 0.4834 | -691.0 | -605.9 | |
| 0 | 4 | 0 | 2 | 23.26 | 246.80 | 23.82 | 312.53 | 0.5056 | -661.0 | -650.1 | |
| 0 | 11 | 0 | 6 | 19.99 | 246.19 | 23.21 | 307.68 | 0.4699 | -1057.0 | -846.3 | |
| 0 | 9 | 0 | 5 | 20.16 | 245.86 | 22.88 | 308.35 | 0.4673 | -864.0 | -834.0 | |
| 0 | 5 | 0 | 3 | 19.85 | 245.50 | 22.52 | 308.18 | 0.4603 | -1114.0 | -972.9 | |
| 0 | 4 | 0 | 2 | 20.21 | 245.51 | 22.53 | 308.82 | 0.4635 | -1012.0 | -944.2 | |
| 0 | 6 | 0 | 3 | 20.59 | 244.72 | 21.75 | 310.42 | 0.4575 | -550.0 | -580.9 | |
| 0 | 17 | 0 | 9 | 20.24 | 244.41 | 21.43 | 310.17 | 0.4505 | -805.0 | -962.3 | |
| 0 | 5 | 0 | 3 | 22.54 | 244.59 | 21.61 | 313.93 | 0.4742 | -637.0 | -660.7 | |
| 0 | 6 | 0 | 3 | 18.25 | 243.70 | 20.72 | 307.28 | 0.4242 | -751.0 | -698.3 | |
| 0 | 5 | 0 | 3 | 22.27 | 243.87 | 20.90 | 314.37 | 0.4637 | -670.0 | -662.7 | |
| 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. | |