SDO HMI 2011-05-01 00:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.41 | 167.29 | 44.89 | 353.92 | 20.50 | 186.57 | 73.42 | 292.41 | 0.9697 | 202.1 | 13.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.05 | 32.46 | 7.10 | 109.85 | 20.10 | 192.77 | 79.61 | 291.04 | 0.9903 | 297.7 | -44.2 | |
| 2.68 | -1.00 | 8.74 | -1.00 | 20.03 | 192.27 | 79.12 | 291.03 | 0.9891 | -363.2 | 999999 | |
| 0.00 | 1.43 | 0.00 | 3.24 | 19.51 | 188.20 | 75.04 | 291.07 | 0.9769 | -272.0 | -268.2 | |
| 0.45 | 3.75 | 0.91 | 7.72 | 19.82 | 186.67 | 73.52 | 291.63 | 0.9715 | -68.4 | -44.7 | |
| 0.00 | 2.94 | 0.00 | 6.09 | 20.37 | 186.68 | 73.52 | 292.19 | 0.9719 | -244.0 | -225.1 | |
| 1.34 | 117.26 | 2.40 | 209.97 | 20.56 | 184.31 | 71.15 | 292.80 | 0.9624 | -120.3 | 55.9 | |
| 7.13 | -6.00 | 12.47 | -6.00 | 20.49 | 183.83 | 70.68 | 292.82 | 0.9603 | 434.4 | 999999 | |
| 0.00 | 1.07 | 0.00 | 2.02 | 21.53 | 185.03 | 71.87 | 293.66 | 0.9663 | -366.0 | -351.6 | |
| 3.30 | -6.00 | 5.75 | -6.00 | 20.91 | 183.69 | 70.54 | 293.27 | 0.9600 | 351.6 | 999999 | |
| 0.00 | 1.16 | 0.00 | 2.19 | 22.17 | 184.76 | 71.61 | 294.36 | 0.9658 | -408.0 | -325.7 | |
| 4.46 | -6.00 | 7.52 | -6.00 | 20.80 | 183.09 | 69.94 | 293.28 | 0.9572 | 643.1 | 999999 | |
| 0.00 | 4.64 | 0.00 | 8.47 | 22.07 | 184.33 | 71.18 | 294.34 | 0.9639 | 43.0 | 57.0 | |
| 0.00 | 1.69 | 0.00 | 2.85 | 21.57 | 182.87 | 69.72 | 294.11 | 0.9570 | 522.0 | 443.2 | |
| 0.00 | 0.89 | 0.00 | 1.52 | 21.82 | 183.04 | 69.89 | 294.33 | 0.9580 | 350.0 | 331.8 | |
| 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. | |