SOHO MDI 2000-11-03 16:29:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 88 | 464 | 64 | 340 | -23.38 | 305.37 | 39.63 | 232.71 | 0.7378 | -717.2 | -334.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 70 | 7 | 52 | -22.44 | 307.79 | 42.05 | 235.28 | 0.7554 | -906.6 | -494.1 | |
| 7 | -1 | 5 | -1 | -22.60 | 307.40 | 41.66 | 234.88 | 0.7526 | -993.9 | 999999 | |
| 0 | 4 | 0 | 3 | -22.93 | 306.30 | 40.56 | 233.84 | 0.7440 | -626.0 | -549.8 | |
| 22 | 259 | 17 | 192 | -24.08 | 305.95 | 40.21 | 232.29 | 0.7474 | -1011.4 | -331.6 | |
| 7 | 25 | 5 | 18 | -20.38 | 304.59 | 38.85 | 235.87 | 0.7127 | -615.0 | -556.1 | |
| 0 | 7 | 0 | 5 | -22.61 | 305.10 | 39.35 | 233.47 | 0.7308 | -918.0 | -806.4 | |
| 11 | -4 | 8 | -4 | -24.36 | 305.62 | 39.88 | 231.75 | 0.7461 | -1044.5 | 999999 | |
| 0 | 1 | 0 | 1 | -22.13 | 304.83 | 39.08 | 233.88 | 0.7253 | 226.0 | 200.8 | |
| 4 | -4 | 3 | -4 | -23.57 | 305.27 | 39.53 | 232.45 | 0.7381 | -1067.5 | 999999 | |
| 15 | 42 | 11 | 30 | -22.49 | 304.30 | 38.56 | 233.11 | 0.7224 | -333.3 | -581.4 | |
| 6 | -10 | 4 | -10 | -23.22 | 304.39 | 38.65 | 232.30 | 0.7277 | -904.0 | 999999 | |
| 0 | 7 | 0 | 5 | -22.92 | 303.43 | 37.69 | 232.02 | 0.7167 | -720.0 | -574.6 | |
| 0 | 8 | 0 | 6 | -25.64 | 303.97 | 38.22 | 229.21 | 0.7391 | 608.0 | 466.9 | |
| 0 | 5 | 0 | 3 | -21.21 | 302.33 | 36.59 | 233.36 | 0.6949 | -482.0 | -393.0 | |
| 0 | 4 | 0 | 3 | -22.01 | 302.26 | 36.51 | 232.32 | 0.6994 | -281.0 | -324.7 | |
| 0 | 3 | 0 | 2 | -22.31 | 302.19 | 36.45 | 231.91 | 0.7007 | -459.0 | -406.4 | |
| 0 | 3 | 0 | 2 | -25.52 | 302.20 | 36.46 | 228.13 | 0.7224 | 407.0 | 374.5 | |
| 7 | 26 | 4 | 18 | -22.50 | 299.59 | 33.85 | 229.76 | 0.6765 | 921.4 | 607.2 | |
| 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. | |