SDO HMI 2012-05-08 06:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.34 | 21.49 | 0.70 | 11.29 | 15.77 | 227.91 | 1.36 | 355.37 | 0.3368 | -304.1 | -308.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.70 | 0.00 | 0.89 | 13.81 | 235.66 | 9.11 | 332.44 | 0.3338 | -891.0 | -717.8 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 12.89 | 235.18 | 8.63 | 332.35 | 0.3167 | -739.0 | -585.1 | |
| 0.00 | 1.52 | 0.00 | 0.82 | 19.12 | 231.17 | 4.62 | 348.74 | 0.3915 | -837.0 | -631.5 | |
| 0.00 | 1.25 | 0.00 | 0.65 | 14.09 | 230.89 | 4.34 | 346.23 | 0.3101 | -807.0 | -623.6 | |
| 1.34 | 3.76 | 0.70 | 1.95 | 13.68 | 229.61 | 3.06 | 349.97 | 0.2989 | -1139.8 | -928.6 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 13.87 | 229.58 | 3.03 | 350.18 | 0.3019 | -669.0 | -494.4 | |
| 0.00 | 2.06 | 0.00 | 1.07 | 14.69 | 227.40 | 0.85 | 357.35 | 0.3116 | -866.0 | -668.1 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 16.45 | 226.84 | 0.29 | 359.19 | 0.3405 | -728.0 | -524.0 | |
| 0.00 | 1.61 | 0.00 | 0.85 | 16.06 | 226.18 | -0.37 | 1.08 | 0.3342 | -735.0 | -589.3 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 17.62 | 223.28 | -3.27 | 8.63 | 0.3637 | 750.0 | 612.5 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 17.85 | 222.96 | -3.59 | 9.36 | 0.3682 | 878.0 | 726.9 | |
| 0.00 | 2.69 | 0.00 | 1.43 | 17.94 | 222.83 | -3.72 | 9.64 | 0.3701 | 773.0 | 428.9 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 18.27 | 222.22 | -4.33 | 11.02 | 0.3771 | 807.0 | 643.2 | |
| 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. | |