SDO HMI 2011-06-25 02:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.79 | 53.76 | 20.30 | 57.93 | 17.05 | 166.31 | 61.92 | 288.12 | 0.8892 | -107.8 | -165.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.64 | 0.00 | 0.72 | 15.96 | 167.89 | 63.50 | 286.73 | 0.9003 | -395.0 | -370.9 | |
| 7.45 | 9.99 | 8.38 | 11.23 | 16.63 | 167.79 | 63.40 | 287.48 | 0.9000 | -525.3 | -530.9 | |
| 0.00 | 1.00 | 0.00 | 1.11 | 16.04 | 167.30 | 62.91 | 286.88 | 0.8960 | -672.0 | -596.3 | |
| 0.00 | 1.82 | 0.00 | 2.23 | 19.96 | 169.88 | 65.49 | 290.89 | 0.9171 | 245.0 | 168.9 | |
| 0.00 | 0.36 | 0.00 | 0.40 | 16.17 | 167.17 | 62.77 | 287.04 | 0.8951 | -458.0 | -545.0 | |
| 0.00 | 1.82 | 0.00 | 1.98 | 16.22 | 166.84 | 62.45 | 287.12 | 0.8927 | -538.0 | -518.0 | |
| 0.00 | 3.45 | 0.00 | 3.68 | 16.24 | 166.17 | 61.78 | 287.23 | 0.8876 | -284.0 | -300.2 | |
| 1.54 | 3.18 | 1.63 | 3.36 | 16.05 | 165.93 | 61.54 | 287.05 | 0.8856 | 207.0 | 167.7 | |
| 0.00 | 1.00 | 0.00 | 1.13 | 19.29 | 167.57 | 63.18 | 290.45 | 0.9008 | -296.0 | -296.6 | |
| 0.00 | 2.81 | 0.00 | 2.98 | 16.69 | 165.88 | 61.49 | 287.77 | 0.8857 | -201.0 | -215.7 | |
| 1.63 | 25.51 | 1.72 | 26.93 | 17.08 | 165.69 | 61.30 | 288.23 | 0.8847 | -276.6 | -89.3 | |
| 0.00 | 1.18 | 0.00 | 1.26 | 17.80 | 165.98 | 61.59 | 289.00 | 0.8876 | 189.0 | 126.8 | |
| 5.99 | -11.00 | 6.27 | -11.00 | 17.12 | 165.45 | 61.06 | 288.30 | 0.8828 | 445.1 | 999999 | |
| 2.18 | -11.00 | 2.30 | -11.00 | 17.49 | 165.66 | 61.27 | 288.70 | 0.8849 | 294.6 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.92 | 19.22 | 160.39 | 56.00 | 291.55 | 0.8437 | 216.0 | 231.2 | |
| 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. | |