SDO HMI 2011-08-06 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.60 | 24.15 | 3.69 | 15.76 | 18.98 | 223.10 | -39.53 | 67.78 | 0.6515 | -92.7 | -151.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.93 | 17.94 | 229.27 | -33.36 | 67.06 | 0.5702 | -751.0 | -562.0 | |
| 0.00 | 1.63 | 0.00 | 1.02 | 19.79 | 226.64 | -35.99 | 65.20 | 0.6113 | -844.0 | -636.2 | |
| 0.00 | 1.36 | 0.00 | 0.86 | 20.45 | 225.53 | -37.10 | 64.66 | 0.6276 | -334.0 | -451.4 | |
| 0.00 | 1.36 | 0.00 | 0.86 | 20.31 | 225.28 | -37.34 | 64.98 | 0.6301 | -690.0 | -480.1 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 21.34 | 224.48 | -38.14 | 63.76 | 0.6437 | -508.0 | -399.5 | |
| 0.00 | 1.18 | 0.00 | 0.73 | 14.56 | 225.73 | -36.89 | 73.94 | 0.6069 | 723.0 | 588.5 | |
| 2.89 | 6.24 | 1.87 | 4.02 | 17.94 | 223.67 | -38.95 | 69.19 | 0.6421 | -717.2 | -599.4 | |
| 0.81 | 1.90 | 0.53 | 1.23 | 18.38 | 223.18 | -39.44 | 68.68 | 0.6495 | -562.4 | -585.6 | |
| 0.00 | 0.99 | 0.00 | 0.67 | 19.16 | 220.70 | -41.92 | 68.29 | 0.6816 | 743.0 | 609.2 | |
| 0.00 | 0.72 | 0.00 | 0.49 | 19.21 | 220.55 | -42.07 | 68.26 | 0.6835 | 535.0 | 506.9 | |
| 0.00 | 2.26 | 0.00 | 1.53 | 18.89 | 220.48 | -42.14 | 68.74 | 0.6835 | 661.0 | 531.7 | |
| 1.90 | 2.35 | 1.29 | 1.59 | 18.81 | 220.33 | -42.29 | 68.89 | 0.6851 | 451.4 | 424.4 | |
| 0.00 | 1.08 | 0.00 | 0.84 | 23.34 | 213.82 | -48.81 | 64.50 | 0.7677 | 253.0 | 258.6 | |
| 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. | |