SDO HMI 2011-08-11 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.07 | 30.38 | 8.45 | 18.39 | -21.85 | 172.95 | -20.79 | 145.02 | 0.5744 | 61.8 | 123.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.75 | -24.31 | 179.11 | -14.63 | 155.63 | 0.5599 | -579.0 | -532.1 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -18.59 | 175.66 | -18.09 | 144.84 | 0.5131 | 702.0 | 585.8 | |
| 3.97 | 12.09 | 2.35 | 7.16 | -20.95 | 174.79 | -18.95 | 146.28 | 0.5485 | 955.4 | 644.7 | |
| 4.15 | -3.00 | 2.46 | -3.00 | -21.07 | 174.53 | -19.21 | 146.05 | 0.5519 | 755.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -20.63 | 174.42 | -19.32 | 145.41 | 0.5477 | 624.0 | 471.8 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -20.98 | 174.27 | -19.47 | 145.59 | 0.5530 | 512.0 | 464.2 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -19.25 | 173.23 | -20.52 | 142.22 | 0.5422 | 559.0 | 319.8 | |
| 5.95 | 7.22 | 3.64 | 4.42 | -22.88 | 172.48 | -21.26 | 145.30 | 0.5892 | -858.0 | -664.6 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -22.53 | 172.50 | -21.24 | 144.97 | 0.5851 | -734.0 | -576.9 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -22.43 | 172.38 | -21.37 | 144.70 | 0.5850 | -613.0 | -477.4 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -24.58 | 171.93 | -21.81 | 146.38 | 0.6124 | -696.0 | -624.6 | |
| 0.00 | 1.71 | 0.00 | 1.10 | -22.33 | 165.99 | -27.75 | 137.46 | 0.6394 | 932.0 | 696.8 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -23.88 | 161.60 | -32.15 | 135.16 | 0.6922 | -549.0 | -365.8 | |
| 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. | |