SOHO MDI 2000-07-16 17:01:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 220 | 27 | 115 | 20.49 | 288.52 | 10.21 | 329.35 | 0.3246 | 579.9 | 110.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 10 | 0 | 6 | 27.25 | 297.23 | 18.92 | 323.49 | 0.4865 | -649.0 | -575.0 | |
| 0 | 5 | 0 | 3 | 21.27 | 293.45 | 15.14 | 319.99 | 0.3802 | 929.0 | 836.3 | |
| 0 | 3 | 0 | 1 | 21.48 | 293.20 | 14.90 | 320.81 | 0.3802 | 604.0 | 666.6 | |
| 0 | 5 | 0 | 3 | 24.74 | 293.13 | 14.82 | 326.21 | 0.4196 | 714.0 | 686.8 | |
| 22 | 91 | 11 | 47 | 19.69 | 289.62 | 11.31 | 324.85 | 0.3222 | 1141.8 | 727.8 | |
| 17 | -5 | 9 | -5 | 18.88 | 289.48 | 11.17 | 323.59 | 0.3102 | 1418.4 | 999999 | |
| 0 | 4 | 0 | 2 | 20.61 | 288.74 | 10.43 | 328.58 | 0.3266 | 460.0 | 373.8 | |
| 0 | 18 | 0 | 9 | 19.31 | 287.80 | 9.50 | 328.63 | 0.3005 | -512.0 | -194.5 | |
| 0 | 5 | 0 | 3 | 18.67 | 286.84 | 8.53 | 330.10 | 0.2831 | -795.0 | -638.1 | |
| 0 | 3 | 0 | 2 | 20.47 | 286.85 | 8.54 | 333.14 | 0.3093 | -502.0 | -407.1 | |
| 0 | 5 | 0 | 3 | 19.08 | 286.01 | 7.71 | 333.24 | 0.2827 | 735.0 | 619.9 | |
| 5 | 35 | 2 | 18 | 21.47 | 285.92 | 7.61 | 337.06 | 0.3177 | -1199.1 | -746.2 | |
| 0 | 5 | 0 | 2 | 19.13 | 285.55 | 7.24 | 334.69 | 0.2799 | 363.0 | 462.5 | |
| 9 | -12 | 5 | -12 | 21.51 | 285.53 | 7.23 | 338.15 | 0.3160 | -1168.4 | 999999 | |
| 0 | 15 | 0 | 8 | 20.20 | 285.34 | 7.04 | 336.92 | 0.2947 | -502.0 | -311.2 | |
| 0 | 16 | 0 | 8 | 21.15 | 284.88 | 6.57 | 339.52 | 0.3064 | -1023.0 | -805.1 | |
| 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. | |