SDO HMI 2011-08-05 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.45 | 19.45 | 1.51 | 11.99 | 18.54 | 241.83 | -35.12 | 66.63 | 0.5957 | 110.5 | 119.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.89 | 0.00 | 1.69 | 18.45 | 246.50 | -30.45 | 64.59 | 0.5343 | -828.0 | -607.6 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 17.97 | 245.74 | -31.21 | 65.86 | 0.5423 | -817.0 | -649.3 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 17.98 | 245.36 | -31.59 | 66.03 | 0.5474 | -817.0 | -610.3 | |
| 1.27 | 1.45 | 0.77 | 0.88 | 18.23 | 243.10 | -33.86 | 66.70 | 0.5783 | -635.7 | -538.5 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 19.73 | 241.21 | -35.74 | 65.12 | 0.6084 | 506.0 | 320.4 | |
| 0.00 | 1.72 | 0.00 | 1.08 | 19.88 | 240.61 | -36.35 | 65.14 | 0.6165 | 639.0 | 558.3 | |
| 1.18 | 1.18 | 0.74 | 0.74 | 19.08 | 240.33 | -36.62 | 66.52 | 0.6169 | 765.3 | 0.0 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 19.44 | 240.08 | -36.87 | 66.05 | 0.6214 | 581.0 | 510.5 | |
| 0.00 | 1.90 | 0.00 | 1.20 | 19.25 | 240.09 | -36.86 | 66.34 | 0.6206 | 555.0 | 527.2 | |
| 0.00 | 1.18 | 0.00 | 0.74 | 18.13 | 240.33 | -36.62 | 68.00 | 0.6136 | 629.0 | 478.1 | |
| 0.00 | 2.53 | 0.00 | 1.59 | 18.62 | 240.01 | -36.94 | 67.37 | 0.6193 | 768.0 | 692.5 | |
| 0.00 | 0.99 | 0.00 | 0.63 | 18.12 | 239.61 | -37.34 | 68.29 | 0.6227 | 640.0 | 527.1 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 14.72 | 236.21 | -40.74 | 74.47 | 0.6574 | -551.0 | -427.4 | |
| 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. | |