SDO HMI 2011-01-05 02:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.32 | 401.72 | 42.98 | 248.77 | 31.34 | 188.40 | -12.62 | 18.14 | 0.6015 | -978.3 | -361.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.30 | 29.33 | 196.16 | -4.87 | 7.78 | 0.5486 | -522.0 | -579.5 | |
| 0.00 | 1.61 | 0.00 | 0.96 | 29.65 | 195.98 | -5.05 | 7.98 | 0.5536 | -746.0 | -655.6 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 29.19 | 195.80 | -5.23 | 8.40 | 0.5474 | -797.0 | -648.5 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 30.23 | 194.27 | -6.76 | 10.40 | 0.5658 | -612.0 | -524.2 | |
| 0.00 | 0.93 | 0.00 | 0.56 | 29.73 | 191.25 | -9.78 | 15.11 | 0.5684 | -497.0 | -415.9 | |
| 0.00 | 1.10 | 0.00 | 0.74 | 37.84 | 189.68 | -11.34 | 13.26 | 0.6795 | 705.0 | 606.7 | |
| 65.16 | 381.36 | 40.27 | 235.89 | 31.26 | 188.41 | -12.61 | 18.19 | 0.6004 | -1318.4 | -375.9 | |
| 0.00 | 1.78 | 0.00 | 1.17 | 35.14 | 187.24 | -13.79 | 17.39 | 0.6546 | 724.0 | 658.0 | |
| 0.00 | 1.95 | 0.00 | 1.26 | 34.17 | 186.74 | -14.29 | 18.54 | 0.6447 | -664.0 | -451.4 | |
| 0.00 | 0.93 | 0.00 | 0.60 | 33.87 | 186.64 | -14.39 | 18.83 | 0.6414 | -599.0 | -442.3 | |
| 0.00 | 1.10 | 0.00 | 0.66 | 28.21 | 187.08 | -13.95 | 22.09 | 0.5671 | -677.0 | -486.5 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 30.11 | 186.29 | -14.74 | 21.77 | 0.5959 | 390.0 | 331.8 | |
| 4.16 | 5.78 | 2.71 | 3.76 | 34.16 | 185.12 | -15.91 | 20.45 | 0.6518 | 795.1 | 537.0 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 33.79 | 181.31 | -19.72 | 24.96 | 0.6668 | 446.0 | 394.1 | |
| 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. | |