SOHO MDI 2000-11-04 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38 | 287 | 40 | 288 | -23.50 | 305.43 | 55.22 | 240.08 | 0.8706 | -558.5 | -187.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 35 | 13 | 37 | -22.56 | 307.78 | 57.57 | 241.89 | 0.8857 | -577.6 | -231.8 | |
| 2 | 10 | 2 | 10 | -20.48 | 306.06 | 55.85 | 243.61 | 0.8676 | -325.0 | -371.4 | |
| 0 | 4 | 0 | 3 | -20.30 | 305.09 | 54.88 | 243.49 | 0.8594 | -351.0 | -364.7 | |
| 0 | 3 | 0 | 3 | -20.56 | 304.66 | 54.45 | 243.05 | 0.8567 | -220.0 | -221.4 | |
| 0 | 2 | 0 | 2 | -20.22 | 304.48 | 54.27 | 243.37 | 0.8543 | -617.0 | -543.4 | |
| 23 | 185 | 24 | 189 | -24.18 | 306.24 | 56.03 | 239.63 | 0.8788 | -632.4 | -196.6 | |
| 0 | 2 | 0 | 2 | -22.93 | 305.36 | 55.15 | 240.68 | 0.8689 | -459.0 | -382.8 | |
| -6 | -6 | -6 | -6 | -24.32 | 305.57 | 55.36 | 239.26 | 0.8744 | 999999 | 999999 | |
| 0 | 7 | 0 | 7 | -23.40 | 304.55 | 54.34 | 239.89 | 0.8641 | -510.0 | -413.5 | |
| 0 | 7 | 0 | 6 | -20.38 | 302.82 | 52.62 | 242.61 | 0.8411 | -602.0 | -568.8 | |
| 0 | 3 | 0 | 3 | -20.70 | 302.65 | 52.44 | 242.18 | 0.8406 | -541.0 | -466.2 | |
| 0 | 4 | 0 | 4 | -20.66 | 301.95 | 51.75 | 241.96 | 0.8347 | -582.0 | -514.4 | |
| 0 | 5 | 0 | 4 | -21.84 | 300.35 | 50.14 | 239.99 | 0.8250 | 228.0 | 238.6 | |
| 0 | 7 | 0 | 6 | -22.62 | 299.82 | 49.61 | 238.89 | 0.8234 | 400.0 | 408.8 | |
| 1 | 13 | 1 | 12 | -23.42 | 298.80 | 48.60 | 237.55 | 0.8179 | 530.0 | 447.2 | |
| 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. | |