SDO HMI 2011-05-03 20:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.09 | 314.19 | 26.94 | 172.96 | 17.80 | 61.61 | -14.11 | 32.12 | 0.4372 | -644.4 | -346.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.80 | 0.00 | 0.44 | 18.24 | 64.90 | -10.81 | 25.34 | 0.4181 | -747.0 | -585.1 | |
| 0.00 | 2.59 | 0.00 | 1.40 | 17.18 | 64.39 | -11.33 | 27.61 | 0.4067 | 743.0 | 521.9 | |
| 49.09 | 293.76 | 26.94 | 161.14 | 17.60 | 61.96 | -13.76 | 31.83 | 0.4317 | -1246.8 | -426.1 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 20.05 | 57.70 | -18.02 | 35.77 | 0.4991 | 832.0 | 726.6 | |
| 0.00 | 3.03 | 0.00 | 1.72 | 18.39 | 56.91 | -18.80 | 39.10 | 0.4869 | 619.0 | 673.5 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 18.79 | 56.60 | -19.12 | 39.01 | 0.4945 | 791.0 | 658.4 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 24.83 | 55.31 | -20.41 | 33.55 | 0.5748 | 731.0 | 630.3 | |
| 0.00 | 2.14 | 0.00 | 1.22 | 18.21 | 56.16 | -19.56 | 40.43 | 0.4923 | 793.0 | 701.1 | |
| 0.00 | 1.61 | 0.00 | 0.96 | 23.36 | 55.06 | -20.66 | 35.47 | 0.5602 | 727.0 | 662.9 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 20.23 | 55.42 | -20.29 | 38.75 | 0.5219 | 638.0 | 615.2 | |
| 0.00 | 1.61 | 0.00 | 0.97 | 24.09 | 54.73 | -20.99 | 35.08 | 0.5712 | 697.0 | 464.3 | |
| 0.00 | 2.05 | 0.00 | 1.19 | 20.07 | 55.34 | -20.37 | 39.07 | 0.5208 | 598.0 | 534.7 | |
| 0.00 | 1.43 | 0.00 | 0.86 | 23.23 | 53.63 | -22.08 | 37.40 | 0.5710 | 797.0 | 734.2 | |
| 0.00 | 2.05 | 0.00 | 1.24 | 23.44 | 53.45 | -22.26 | 37.37 | 0.5748 | 633.0 | 470.2 | |
| 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. | |