SDO HMI 2011-06-02 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.36 | 172.49 | 19.74 | 101.69 | -20.60 | 19.27 | -26.81 | 129.18 | 0.5466 | 598.7 | 425.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.83 | -20.34 | 23.32 | -22.76 | 133.09 | 0.4987 | -702.0 | -560.3 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -20.15 | 23.35 | -22.73 | 132.82 | 0.4966 | -747.0 | -637.2 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -18.48 | 23.59 | -22.49 | 130.38 | 0.4781 | -611.0 | -552.4 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -19.43 | 22.26 | -23.82 | 130.43 | 0.5023 | -901.0 | -688.1 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -18.92 | 21.74 | -24.34 | 129.03 | 0.5038 | -730.0 | -535.0 | |
| 24.41 | 153.05 | 14.40 | 90.16 | -20.52 | 19.39 | -26.69 | 129.16 | 0.5446 | 1173.7 | 494.6 | |
| 4.61 | -6.00 | 2.74 | -6.00 | -20.84 | 18.74 | -27.34 | 129.03 | 0.5546 | 748.7 | 999999 | |
| 3.07 | 6.60 | 1.84 | 3.95 | -21.40 | 18.41 | -27.67 | 129.54 | 0.5628 | 692.0 | 550.1 | |
| 1.27 | -8.00 | 0.76 | -8.00 | -21.13 | 18.31 | -27.77 | 129.06 | 0.5618 | 557.2 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -19.61 | 18.54 | -27.54 | 126.96 | 0.5472 | -364.0 | -294.2 | |
| 0.00 | 2.44 | 0.00 | 1.46 | -20.84 | 18.26 | -27.82 | 128.58 | 0.5600 | 704.0 | 530.1 | |
| 0.00 | 0.90 | 0.00 | 0.56 | -22.30 | 16.07 | -30.01 | 128.79 | 0.5958 | 493.0 | 442.4 | |
| 0.00 | 1.90 | 0.00 | 1.22 | -23.08 | 12.29 | -33.79 | 126.93 | 0.6424 | -586.0 | -452.4 | |
| 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. | |