SDO HMI 2011-05-30 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.58 | 99.62 | 13.40 | 67.49 | 15.68 | 40.08 | -40.19 | 65.59 | 0.6841 | -183.5 | -219.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.57 | 21.36 | 49.04 | -31.23 | 52.06 | 0.6145 | 484.0 | 410.1 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 18.83 | 45.15 | -35.12 | 58.43 | 0.6413 | 603.0 | 564.7 | |
| 0.00 | 0.63 | 0.00 | 0.42 | 16.37 | 41.17 | -39.10 | 64.15 | 0.6747 | -613.0 | -501.7 | |
| 14.35 | 73.11 | 9.58 | 48.72 | 15.39 | 40.99 | -39.28 | 65.61 | 0.6725 | -1008.0 | -392.4 | |
| 0.00 | 3.16 | 0.00 | 2.14 | 15.49 | 40.19 | -40.08 | 65.84 | 0.6824 | -489.0 | -398.2 | |
| 0.00 | 1.62 | 0.00 | 1.10 | 15.21 | 39.80 | -40.47 | 66.40 | 0.6858 | -629.0 | -468.9 | |
| 0.00 | 1.35 | 0.00 | 0.93 | 15.32 | 38.73 | -41.54 | 66.72 | 0.6986 | 711.0 | 558.8 | |
| 0.00 | 1.44 | 0.00 | 1.04 | 17.02 | 36.76 | -43.51 | 65.26 | 0.7271 | 669.0 | 534.8 | |
| 0.00 | 1.44 | 0.00 | 1.03 | 15.85 | 36.79 | -43.48 | 66.80 | 0.7225 | 765.0 | 575.4 | |
| 0.00 | 2.35 | 0.00 | 1.68 | 15.75 | 36.55 | -43.72 | 67.02 | 0.7249 | 530.0 | 472.2 | |
| 0.00 | 1.53 | 0.00 | 1.11 | 16.11 | 36.28 | -43.99 | 66.66 | 0.7291 | 280.0 | 296.1 | |
| 0.00 | 1.26 | 0.00 | 0.92 | 16.33 | 35.95 | -44.33 | 66.49 | 0.7335 | 596.0 | 560.1 | |
| 1.44 | 9.75 | 1.05 | 7.13 | 16.49 | 35.72 | -44.55 | 66.37 | 0.7365 | 605.7 | 339.2 | |
| 3.79 | -13.00 | 2.77 | -13.00 | 16.65 | 35.63 | -44.64 | 66.19 | 0.7381 | 590.4 | 999999 | |
| 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. | |