SOHO MDI 2000-09-23 15:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89 | 523 | 44 | 265 | -5.74 | 82.88 | -3.72 | 164.62 | 0.2349 | -300.9 | -144.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 292 | 9 | 148 | -5.00 | 85.93 | -0.67 | 176.77 | 0.2089 | -1690.2 | -692.3 | |
| 10 | -1 | 5 | -1 | -5.36 | 85.46 | -1.14 | 174.69 | 0.2157 | -1469.2 | 999999 | |
| 6 | -1 | 3 | -1 | -5.60 | 85.26 | -1.34 | 173.90 | 0.2201 | -1558.3 | 999999 | |
| 10 | -1 | 5 | -1 | -5.96 | 84.87 | -1.73 | 172.35 | 0.2270 | -1402.1 | 999999 | |
| 4 | -1 | 2 | -1 | -6.08 | 84.28 | -2.32 | 169.90 | 0.2306 | -982.6 | 999999 | |
| 4 | -1 | 2 | -1 | -5.84 | 83.69 | -2.91 | 167.19 | 0.2287 | -1128.2 | 999999 | |
| 0 | 24 | 0 | 12 | -6.25 | 83.18 | -3.42 | 165.46 | 0.2374 | -797.0 | -616.2 | |
| 0 | 7 | 0 | 4 | -5.81 | 82.79 | -3.81 | 163.36 | 0.2320 | -615.0 | -597.3 | |
| 0 | 4 | 0 | 2 | -6.21 | 82.71 | -3.89 | 163.52 | 0.2389 | -317.0 | -357.7 | |
| 0 | 4 | 0 | 2 | -6.18 | 81.72 | -4.88 | 159.62 | 0.2437 | -373.0 | -279.0 | |
| 14 | 85 | 7 | 43 | -6.52 | 80.26 | -6.34 | 154.78 | 0.2585 | 1389.4 | 776.7 | |
| 0 | 7 | 0 | 3 | -5.72 | 80.08 | -6.52 | 152.72 | 0.2478 | 1355.0 | 1108.4 | |
| 0 | 12 | 0 | 6 | -5.45 | 79.76 | -6.84 | 151.08 | 0.2461 | 945.0 | 854.6 | |
| 9 | -11 | 4 | -11 | -6.77 | 79.31 | -7.29 | 152.00 | 0.2696 | 1112.9 | 999999 | |
| 8 | 88 | 4 | 45 | -5.71 | 78.61 | -7.99 | 147.69 | 0.2598 | 1565.3 | 742.3 | |
| 6 | -15 | 3 | -15 | -5.59 | 78.30 | -8.30 | 146.43 | 0.2610 | 1461.7 | 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. | |