SOHO MDI 1999-04-12 01:35:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44 | 260 | 22 | 144 | -18.17 | 233.12 | -20.65 | 123.26 | 0.4015 | -228.8 | 78.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 1 | 0 | 1 | -18.37 | 239.06 | -14.71 | 132.25 | 0.3271 | -477.0 | -415.3 | |
| 0 | 8 | 0 | 4 | -16.21 | 237.39 | -16.39 | 124.02 | 0.3284 | -1010.0 | -908.7 | |
| 2 | 12 | 1 | 6 | -16.53 | 237.23 | -16.54 | 124.60 | 0.3331 | -1132.8 | -726.5 | |
| 16 | 79 | 8 | 42 | -17.32 | 235.92 | -17.86 | 124.69 | 0.3576 | -1684.0 | -1024.9 | |
| 4 | -4 | 2 | -4 | -16.91 | 235.53 | -18.25 | 123.18 | 0.3594 | -1325.5 | 999999 | |
| 0 | 4 | 0 | 2 | -18.14 | 235.23 | -18.55 | 125.66 | 0.3737 | -862.0 | -653.2 | |
| 4 | 11 | 2 | 6 | -17.08 | 234.48 | -19.30 | 122.24 | 0.3751 | -1073.1 | -720.4 | |
| 0 | 10 | 0 | 6 | -17.55 | 233.12 | -20.65 | 121.75 | 0.3972 | -707.0 | -763.7 | |
| 0 | 10 | 0 | 6 | -18.67 | 232.01 | -21.76 | 122.97 | 0.4205 | 948.0 | 691.0 | |
| 0 | 3 | 0 | 2 | -18.62 | 231.75 | -22.02 | 122.59 | 0.4236 | 907.0 | 759.1 | |
| 0 | 5 | 0 | 3 | -20.01 | 231.42 | -22.36 | 125.08 | 0.4386 | 782.0 | 710.8 | |
| 0 | 12 | 0 | 7 | -17.38 | 231.70 | -22.08 | 119.87 | 0.4155 | 1393.0 | 1099.3 | |
| 2 | 13 | 1 | 7 | -20.36 | 230.87 | -22.91 | 125.17 | 0.4483 | 936.2 | 900.2 | |
| 4 | 68 | 2 | 38 | -19.55 | 230.77 | -23.01 | 123.47 | 0.4434 | 1311.4 | 934.5 | |
| 6 | 14 | 3 | 8 | -18.26 | 230.82 | -22.95 | 120.91 | 0.4335 | 1113.3 | 932.9 | |
| 3 | -14 | 1 | -14 | -18.90 | 230.60 | -23.18 | 121.99 | 0.4409 | 1276.3 | 999999 | |
| 3 | -14 | 2 | -14 | -19.25 | 230.28 | -23.50 | 122.38 | 0.4477 | 741.4 | 999999 | |
| 0 | 6 | 0 | 4 | -18.41 | 230.40 | -23.38 | 120.80 | 0.4401 | 727.0 | 534.8 | |
| 0 | 4 | 0 | 2 | -19.64 | 229.99 | -23.79 | 122.88 | 0.4542 | 721.0 | 562.4 | |
| 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. | |