SOHO MDI 2000-09-22 01:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63 | 254 | 36 | 146 | -5.58 | 80.66 | -27.06 | 114.55 | 0.4993 | -459.4 | -22.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 57 | 10 | 32 | -5.92 | 84.03 | -23.69 | 118.17 | 0.4552 | -1349.2 | -794.4 | |
| 6 | -1 | 3 | -1 | -5.54 | 83.74 | -23.97 | 117.13 | 0.4563 | -1209.1 | 999999 | |
| 3 | 6 | 2 | 3 | -5.84 | 83.30 | -24.42 | 117.27 | 0.4646 | -736.8 | -685.2 | |
| 0 | 1 | 0 | 1 | -5.93 | 83.04 | -24.68 | 117.19 | 0.4688 | -837.0 | -801.1 | |
| 0 | 4 | 0 | 2 | -6.84 | 82.60 | -25.12 | 118.44 | 0.4813 | -558.0 | -442.2 | |
| 15 | 36 | 8 | 20 | -6.16 | 82.50 | -25.21 | 117.10 | 0.4777 | -1104.0 | -614.8 | |
| 3 | 12 | 2 | 7 | -6.63 | 81.91 | -25.80 | 117.41 | 0.4890 | -740.7 | -528.8 | |
| 0 | 4 | 0 | 2 | -6.25 | 81.58 | -26.13 | 116.41 | 0.4908 | -326.0 | -274.8 | |
| 0 | 4 | 0 | 3 | -3.76 | 81.12 | -26.59 | 111.34 | 0.4815 | 510.0 | 469.9 | |
| 0 | 4 | 0 | 3 | -4.06 | 80.85 | -26.86 | 111.69 | 0.4871 | 473.0 | 367.5 | |
| 0 | 2 | 0 | 1 | -5.28 | 79.03 | -28.69 | 112.54 | 0.5196 | 820.0 | 756.2 | |
| 0 | 11 | 0 | 6 | -5.76 | 78.96 | -28.76 | 113.34 | 0.5235 | 734.0 | 704.5 | |
| 7 | 113 | 4 | 66 | -5.07 | 78.50 | -29.22 | 111.78 | 0.5257 | 1290.8 | 530.2 | |
| 7 | -13 | 4 | -13 | -5.49 | 78.21 | -29.51 | 112.30 | 0.5320 | 885.7 | 999999 | |
| 4 | -13 | 3 | -13 | -5.14 | 78.04 | -29.67 | 111.58 | 0.5323 | 951.8 | 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. | |