SDO HMI 2011-06-01 10:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.44 | 178.35 | 22.83 | 119.14 | -20.44 | 19.54 | -38.13 | 120.50 | 0.6736 | 434.3 | 344.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.40 | -19.90 | 23.08 | -34.58 | 121.84 | 0.6305 | -602.0 | -517.1 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -19.58 | 22.89 | -34.78 | 121.25 | 0.6309 | -661.0 | -520.9 | |
| 5.15 | 7.50 | 3.29 | 4.80 | -19.12 | 22.37 | -35.30 | 120.28 | 0.6344 | -689.2 | -530.0 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -19.70 | 22.15 | -35.52 | 120.97 | 0.6402 | -428.0 | -381.7 | |
| 0.00 | 0.99 | 0.00 | 0.64 | -18.22 | 21.68 | -35.99 | 118.57 | 0.6378 | -658.0 | -468.4 | |
| 2.08 | 2.80 | 1.34 | 1.80 | -18.60 | 21.55 | -36.12 | 119.05 | 0.6413 | -693.6 | -524.1 | |
| 21.42 | 157.95 | 14.29 | 105.58 | -20.40 | 19.65 | -38.02 | 120.50 | 0.6723 | 1045.4 | 399.4 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -21.92 | 19.01 | -38.66 | 122.21 | 0.6872 | 506.0 | 284.8 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -21.23 | 18.85 | -38.82 | 121.20 | 0.6854 | 471.0 | 390.9 | |
| 3.89 | -7.00 | 2.62 | -7.00 | -20.72 | 18.97 | -38.70 | 120.56 | 0.6815 | 715.7 | 999999 | |
| 1.90 | -7.00 | 1.29 | -7.00 | -20.91 | 18.62 | -39.05 | 120.64 | 0.6863 | 600.4 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.32 | -22.89 | 16.08 | -41.58 | 121.93 | 0.7228 | 587.0 | 483.6 | |
| 0.00 | 0.81 | 0.00 | 0.58 | -22.23 | 16.11 | -41.56 | 121.10 | 0.7195 | 520.0 | 403.9 | |
| 0.00 | 2.89 | 0.00 | 2.15 | -22.34 | 13.27 | -44.40 | 119.93 | 0.7490 | -301.0 | -279.1 | |
| 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. | |