SDO HMI 2011-05-30 12:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.39 | 99.48 | 16.93 | 70.70 | 15.66 | 39.81 | -43.23 | 66.92 | 0.7187 | -155.6 | -217.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.63 | 0.00 | 1.09 | 18.82 | 45.06 | -37.97 | 60.16 | 0.6737 | 619.0 | 479.8 | |
| 0.45 | 76.65 | 0.31 | 53.64 | 15.57 | 41.08 | -41.96 | 66.54 | 0.7044 | -729.8 | -341.9 | |
| 0.00 | 1.17 | 0.00 | 0.82 | 16.21 | 40.83 | -42.21 | 65.79 | 0.7097 | -633.0 | -531.2 | |
| 0.00 | 1.08 | 0.00 | 0.76 | 16.02 | 40.66 | -42.37 | 66.11 | 0.7108 | -494.0 | -410.9 | |
| 12.82 | -2.00 | 8.97 | -2.00 | 15.39 | 40.65 | -42.38 | 66.97 | 0.7085 | -909.0 | 999999 | |
| 1.63 | -2.00 | 1.15 | -2.00 | 15.61 | 40.16 | -42.87 | 66.86 | 0.7149 | -472.7 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.45 | 15.31 | 38.94 | -44.10 | 67.74 | 0.7276 | 562.0 | 470.4 | |
| 0.00 | 0.90 | 0.00 | 0.65 | 14.59 | 38.46 | -44.57 | 68.86 | 0.7305 | 668.0 | 566.4 | |
| 0.00 | 0.90 | 0.00 | 0.66 | 14.72 | 38.21 | -44.83 | 68.78 | 0.7337 | 460.0 | 473.8 | |
| 0.00 | 1.53 | 0.00 | 1.13 | 15.36 | 37.81 | -45.22 | 68.09 | 0.7401 | 555.0 | 470.8 | |
| 0.45 | 1.99 | 0.34 | 1.49 | 16.86 | 36.95 | -46.08 | 66.46 | 0.7542 | 588.4 | 482.7 | |
| 2.08 | 12.10 | 1.58 | 9.27 | 16.42 | 35.98 | -47.05 | 67.36 | 0.7630 | 755.5 | 550.3 | |
| 5.96 | -12.00 | 4.58 | -12.00 | 16.59 | 35.69 | -47.34 | 67.25 | 0.7665 | 501.4 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.74 | 15.74 | 32.24 | -50.80 | 69.37 | 0.7991 | -552.0 | -488.2 | |
| 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. | |