SDO HMI 2011-05-03 12:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.16 | 310.39 | 23.09 | 174.62 | 17.74 | 61.75 | -18.39 | 39.29 | 0.4755 | -561.1 | -350.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.62 | 294.06 | 22.77 | 164.77 | 17.58 | 62.16 | -17.98 | 38.97 | 0.4698 | -1203.2 | -407.9 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 17.55 | 59.44 | -20.70 | 42.94 | 0.4967 | -807.0 | -660.1 | |
| 0.00 | 0.89 | 0.00 | 0.53 | 19.39 | 56.60 | -23.53 | 43.95 | 0.5448 | 638.0 | 466.1 | |
| 0.00 | 2.23 | 0.00 | 1.31 | 18.57 | 56.66 | -23.48 | 45.01 | 0.5361 | 830.0 | 614.6 | |
| 0.00 | 1.25 | 0.00 | 0.73 | 18.70 | 56.50 | -23.64 | 45.01 | 0.5391 | 604.0 | 527.5 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 18.55 | 56.28 | -23.86 | 45.49 | 0.5399 | 743.0 | 574.9 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 18.19 | 56.08 | -24.05 | 46.21 | 0.5385 | 565.0 | 456.9 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 23.21 | 54.93 | -25.21 | 41.00 | 0.5990 | 425.0 | 566.5 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 20.26 | 55.05 | -25.09 | 44.56 | 0.5691 | 602.0 | 484.8 | |
| 0.00 | 1.87 | 0.00 | 1.18 | 23.43 | 53.41 | -26.72 | 42.32 | 0.6150 | 579.0 | 500.0 | |
| 0.00 | 2.50 | 0.00 | 1.56 | 23.12 | 53.44 | -26.69 | 42.66 | 0.6119 | 758.0 | 681.8 | |
| 0.54 | 2.32 | 0.32 | 1.39 | 18.18 | 53.48 | -26.66 | 49.07 | 0.5664 | 801.5 | 658.0 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 23.33 | 52.47 | -27.66 | 43.39 | 0.6229 | 566.0 | 430.6 | |
| 0.00 | 0.54 | 0.00 | 0.33 | 22.01 | 52.39 | -27.74 | 45.08 | 0.6117 | 585.0 | 527.0 | |
| 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. | |