SDO HMI 2013-03-28 22:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.79 | 247.47 | 24.56 | 132.94 | 15.00 | 255.30 | -6.34 | 16.09 | 0.3860 | -1047.3 | -380.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.74 | 13.28 | 255.83 | -5.80 | 16.08 | 0.3567 | -1027.0 | -835.4 | |
| 26.96 | 234.96 | 14.46 | 126.17 | 15.01 | 255.70 | -5.94 | 15.13 | 0.3844 | -1242.9 | -366.7 | |
| 0.00 | 1.84 | 0.00 | 0.97 | 13.19 | 255.46 | -6.17 | 17.12 | 0.3570 | -986.0 | -735.9 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 12.94 | 255.41 | -6.23 | 17.49 | 0.3533 | -865.0 | -743.5 | |
| 16.90 | -2.00 | 9.07 | -2.00 | 14.99 | 255.07 | -6.56 | 16.65 | 0.3868 | -1181.6 | 999999 | |
| 0.96 | -2.00 | 0.52 | -2.00 | 14.86 | 254.83 | -6.81 | 17.34 | 0.3860 | -940.6 | 999999 | |
| 0.44 | -2.00 | 0.23 | -2.00 | 14.57 | 254.84 | -6.80 | 17.55 | 0.3815 | -890.2 | 999999 | |
| 0.53 | -2.00 | 0.28 | -2.00 | 15.19 | 254.57 | -7.07 | 17.69 | 0.3923 | -719.5 | 999999 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 12.38 | 254.65 | -6.98 | 20.01 | 0.3486 | -859.0 | -700.9 | |
| 0.00 | 1.66 | 0.00 | 0.88 | 12.19 | 254.41 | -7.23 | 20.84 | 0.3471 | -1038.0 | -883.5 | |
| 0.00 | 1.75 | 0.00 | 0.99 | 20.23 | 252.47 | -9.16 | 18.31 | 0.4776 | -759.0 | -573.0 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 11.75 | 252.60 | -9.04 | 26.00 | 0.3522 | -560.0 | -521.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 16.16 | 251.42 | -10.22 | 23.77 | 0.4245 | 739.0 | 557.5 | |
| 0.00 | 1.31 | 0.00 | 0.76 | 22.15 | 249.85 | -11.78 | 21.49 | 0.5184 | -691.0 | -530.9 | |
| 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. | |