SOHO MDI 2000-11-11 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52 | 413 | 27 | 219 | -12.51 | 176.57 | 12.44 | 217.91 | 0.3435 | 1517.3 | 475.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 11 | 0 | 6 | -12.89 | 179.46 | 15.33 | 223.17 | 0.3784 | -900.0 | -693.7 | |
| 8 | 333 | 4 | 176 | -13.27 | 177.57 | 13.44 | 218.80 | 0.3627 | 1287.2 | 703.3 | |
| 14 | -2 | 7 | -2 | -12.19 | 177.39 | 13.26 | 220.42 | 0.3474 | 1950.5 | 999999 | |
| 24 | -2 | 13 | -2 | -12.86 | 177.06 | 12.93 | 218.46 | 0.3524 | 1694.3 | 999999 | |
| -4 | -2 | -4 | -2 | -12.58 | 176.84 | 12.72 | 218.51 | 0.3466 | 999999 | 999999 | |
| 6 | -2 | 3 | -2 | -12.86 | 176.61 | 12.49 | 217.50 | 0.3478 | 1438.9 | 999999 | |
| 0 | 5 | 0 | 2 | -13.65 | 175.85 | 11.72 | 214.42 | 0.3508 | 472.0 | 457.9 | |
| 0 | 3 | 0 | 2 | -13.00 | 175.69 | 11.57 | 215.16 | 0.3408 | 816.0 | 678.1 | |
| 0 | 5 | 0 | 3 | -13.40 | 175.47 | 11.35 | 213.97 | 0.3441 | 802.0 | 711.9 | |
| 0 | 10 | 0 | 5 | -8.68 | 174.77 | 10.65 | 221.80 | 0.2753 | -931.0 | -731.8 | |
| 0 | 13 | 0 | 7 | -9.14 | 173.76 | 9.63 | 217.89 | 0.2703 | -694.0 | -672.5 | |
| 0 | 4 | 0 | 2 | -15.20 | 173.66 | 9.54 | 206.97 | 0.3542 | -771.0 | -662.6 | |
| 0 | 7 | 0 | 4 | -13.26 | 172.98 | 8.85 | 207.97 | 0.3208 | -674.0 | -642.0 | |
| 0 | 13 | 0 | 7 | -12.77 | 172.60 | 8.48 | 207.69 | 0.3109 | -851.0 | -633.5 | |
| 0 | 5 | 0 | 3 | -10.81 | 171.04 | 6.92 | 206.13 | 0.2699 | -838.0 | -716.0 | |
| 0 | 4 | 0 | 2 | -11.99 | 169.57 | 5.45 | 199.56 | 0.2785 | -629.0 | -540.9 | |
| 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. | |