SOHO MDI 2000-09-23 22:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82 | 548 | 40 | 277 | -5.73 | 82.85 | -0.23 | 179.43 | 0.2272 | -179.6 | -89.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 284 | 3 | 144 | -4.82 | 86.31 | 3.23 | 195.38 | 0.2128 | -1491.7 | -759.0 | |
| 13 | -1 | 6 | -1 | -4.93 | 86.00 | 2.92 | 193.82 | 0.2134 | -1636.4 | 999999 | |
| 7 | -1 | 3 | -1 | -5.25 | 85.81 | 2.72 | 192.60 | 0.2179 | -1468.7 | 999999 | |
| 7 | -1 | 3 | -1 | -5.53 | 85.57 | 2.49 | 191.30 | 0.2218 | -1355.0 | 999999 | |
| 10 | -1 | 5 | -1 | -5.89 | 85.18 | 2.10 | 189.30 | 0.2266 | -1312.3 | 999999 | |
| 3 | -1 | 2 | -1 | -6.05 | 84.75 | 1.67 | 187.33 | 0.2282 | -950.3 | 999999 | |
| 0 | 5 | 0 | 2 | -4.93 | 84.24 | 1.16 | 185.57 | 0.2082 | 272.0 | 222.9 | |
| 2 | -1 | 1 | -1 | -5.80 | 84.16 | 1.08 | 184.85 | 0.2230 | -1242.8 | 999999 | |
| 0 | 12 | 0 | 6 | -6.44 | 83.81 | 0.73 | 183.12 | 0.2335 | -875.0 | -748.8 | |
| 0 | 4 | 0 | 2 | -5.80 | 83.50 | 0.41 | 181.86 | 0.2224 | -852.0 | -736.6 | |
| 0 | 9 | 0 | 4 | -5.96 | 83.14 | 0.06 | 180.28 | 0.2250 | -679.0 | -562.0 | |
| 0 | 8 | 0 | 4 | -7.25 | 81.73 | -1.35 | 174.56 | 0.2480 | 691.0 | 450.3 | |
| 0 | 5 | 0 | 3 | -6.45 | 80.55 | -2.53 | 169.31 | 0.2373 | 482.0 | 464.3 | |
| 0 | 40 | 0 | 20 | -5.89 | 80.09 | -2.99 | 166.86 | 0.2296 | 1209.0 | 953.6 | |
| 0 | 12 | 0 | 6 | -5.05 | 80.01 | -3.07 | 165.64 | 0.2160 | 916.0 | 837.4 | |
| 12 | 85 | 6 | 43 | -6.65 | 79.89 | -3.20 | 166.77 | 0.2430 | 1488.3 | 767.4 | |
| 6 | -16 | 3 | -16 | -6.90 | 79.29 | -3.79 | 164.69 | 0.2495 | 1188.2 | 999999 | |
| 8 | 84 | 4 | 43 | -5.74 | 78.64 | -4.45 | 160.67 | 0.2341 | 1573.1 | 746.4 | |
| 7 | -18 | 4 | -18 | -5.55 | 78.36 | -4.72 | 159.28 | 0.2325 | 1494.9 | 999999 | |
| 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. | |