SOHO MDI 1999-04-11 17:35:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44 | 241 | 24 | 136 | -18.11 | 233.35 | -24.82 | 118.91 | 0.4571 | -290.5 | 68.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5 | 11 | 2 | 6 | -16.52 | 237.25 | -20.93 | 119.07 | 0.3935 | -1215.3 | -776.6 | |
| 0 | 3 | 0 | 2 | -17.88 | 236.30 | -21.88 | 121.13 | 0.4161 | -751.0 | -630.6 | |
| 0 | 11 | 0 | 6 | -16.60 | 236.11 | -22.07 | 118.12 | 0.4100 | -651.0 | -413.1 | |
| 14 | 72 | 8 | 39 | -17.39 | 235.92 | -22.26 | 119.68 | 0.4178 | -1583.5 | -982.0 | |
| 3 | -4 | 2 | -4 | -17.33 | 235.48 | -22.69 | 119.14 | 0.4234 | -1237.1 | 999999 | |
| 0 | 3 | 0 | 2 | -18.12 | 235.20 | -22.98 | 120.55 | 0.4326 | -736.0 | -733.6 | |
| 2 | -4 | 1 | -4 | -17.09 | 235.34 | -22.84 | 118.48 | 0.4239 | -1198.5 | 999999 | |
| 0 | 2 | 0 | 1 | -15.19 | 235.39 | -22.78 | 114.28 | 0.4117 | -957.0 | -808.2 | |
| 0 | 6 | 0 | 3 | -17.89 | 234.47 | -23.70 | 119.40 | 0.4410 | -698.0 | -516.8 | |
| 6 | 12 | 3 | 7 | -17.17 | 234.31 | -23.87 | 117.73 | 0.4387 | -908.7 | -470.2 | |
| 0 | 5 | 0 | 3 | -16.76 | 233.11 | -25.07 | 115.92 | 0.4530 | -629.0 | -492.7 | |
| 0 | 7 | 0 | 4 | -18.63 | 232.05 | -26.13 | 118.85 | 0.4784 | 978.0 | 780.7 | |
| 0 | 8 | 0 | 5 | -19.82 | 231.61 | -26.56 | 120.75 | 0.4915 | 1231.0 | 772.9 | |
| 0 | 18 | 0 | 10 | -20.12 | 231.18 | -26.99 | 120.96 | 0.4990 | 1135.0 | 826.3 | |
| 0 | 8 | 0 | 5 | -17.45 | 231.51 | -26.67 | 116.14 | 0.4789 | 955.0 | 1028.7 | |
| 6 | 19 | 4 | 11 | -19.47 | 231.02 | -27.15 | 119.64 | 0.4971 | 1387.9 | 1055.4 | |
| 0 | 3 | 0 | 2 | -19.86 | 230.77 | -27.41 | 120.16 | 0.5028 | 749.0 | 722.4 | |
| 6 | 26 | 3 | 15 | -18.26 | 230.82 | -27.35 | 117.22 | 0.4927 | 1332.1 | 778.4 | |
| 2 | 27 | 1 | 15 | -19.05 | 230.54 | -27.63 | 118.50 | 0.5009 | 1155.7 | 802.1 | |
| 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. | |