SDO HMI 2011-08-10 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.90 | 44.65 | 7.68 | 27.16 | 19.86 | 241.06 | 33.54 | 295.97 | 0.5791 | 427.5 | 145.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.54 | 19.13 | 248.81 | 41.29 | 291.59 | 0.6728 | -660.0 | -602.3 | |
| 0.00 | 2.17 | 0.00 | 1.44 | 19.09 | 248.46 | 40.94 | 291.64 | 0.6685 | -752.0 | -562.1 | |
| 0.00 | 6.23 | 0.00 | 4.00 | 18.37 | 246.12 | 38.60 | 291.30 | 0.6377 | -773.0 | -726.7 | |
| 1.35 | 1.71 | 0.85 | 1.07 | 18.36 | 244.33 | 36.81 | 291.90 | 0.6152 | -661.6 | -555.8 | |
| 0.00 | 1.89 | 0.00 | 1.18 | 18.91 | 243.59 | 36.07 | 293.06 | 0.6076 | -788.0 | -656.3 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 20.01 | 240.52 | 33.01 | 296.26 | 0.5729 | 782.0 | 682.2 | |
| 0.00 | 3.34 | 0.00 | 2.03 | 21.27 | 240.60 | 33.08 | 298.28 | 0.5798 | 705.0 | 629.2 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 21.48 | 240.19 | 32.67 | 298.86 | 0.5757 | 693.0 | 550.2 | |
| 6.95 | 15.25 | 4.10 | 9.01 | 19.68 | 238.62 | 31.10 | 296.74 | 0.5467 | 998.8 | 634.5 | |
| 0.00 | 1.80 | 0.00 | 1.07 | 20.55 | 238.70 | 31.18 | 298.20 | 0.5522 | 824.0 | 668.2 | |
| 4.60 | 6.41 | 2.73 | 3.80 | 20.94 | 238.52 | 31.00 | 298.96 | 0.5519 | 870.3 | 583.0 | |
| 0.00 | 1.80 | 0.00 | 1.07 | 20.74 | 238.10 | 30.58 | 298.89 | 0.5455 | 916.0 | 843.5 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 22.99 | 236.99 | 29.47 | 303.44 | 0.5449 | 703.0 | 523.2 | |
| 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. | |