| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.73 | 69.68 | 12.05 | 38.47 | -15.68 | 114.40 | -22.11 | 124.57 | 0.4415 | 110.2 | 78.3 | |
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back to the solar disc SDO HMI 2011-05-26 11:59:10 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 8.30 | 0.00 | 4.50 | -15.33 | 116.82 | -19.69 | 126.73 | 0.4072 | 1011.0 | 920.3 | |
| 5.23 | 11.18 | 2.85 | 6.08 | -15.76 | 116.51 | -20.00 | 127.21 | 0.4151 | 1036.6 | 778.7 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -16.08 | 116.48 | -20.04 | 127.79 | 0.4183 | 767.0 | 649.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -15.14 | 116.54 | -19.97 | 125.98 | 0.4092 | 757.0 | 629.0 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -16.64 | 116.01 | -20.50 | 128.28 | 0.4293 | 750.0 | 590.0 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -16.82 | 115.31 | -21.20 | 127.74 | 0.4396 | 653.0 | 478.4 | |
| 2.71 | 4.24 | 1.48 | 2.32 | -14.63 | 115.14 | -21.37 | 123.22 | 0.4232 | 877.1 | 703.4 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -15.34 | 115.00 | -21.51 | 124.51 | 0.4309 | 387.0 | 449.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -15.72 | 114.69 | -21.82 | 124.88 | 0.4380 | 528.0 | 444.3 | |
| 0.00 | 2.52 | 0.00 | 1.38 | -14.65 | 114.67 | -21.84 | 122.74 | 0.4297 | 518.0 | 409.5 | |
| 0.00 | 1.80 | 0.00 | 1.00 | -16.31 | 114.35 | -22.17 | 125.63 | 0.4473 | 853.0 | 560.5 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -14.74 | 113.64 | -22.87 | 121.80 | 0.4441 | 601.0 | 463.0 | |
| 0.00 | 5.95 | 0.00 | 3.31 | -15.83 | 113.20 | -23.31 | 123.46 | 0.4582 | -732.0 | -648.2 | |
| 2.61 | 16.59 | 1.46 | 9.25 | -15.45 | 113.01 | -23.50 | 122.54 | 0.4578 | -1032.5 | -849.0 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -16.11 | 112.82 | -23.69 | 123.59 | 0.4652 | -756.0 | -629.9 | |
| 7.75 | 10.10 | 4.35 | 5.66 | -16.29 | 112.56 | -23.95 | 123.66 | 0.4701 | -889.4 | -793.2 | |
| 3.43 | -14.00 | 1.91 | -14.00 | -15.70 | 112.63 | -23.88 | 122.63 | 0.4646 | -818.3 | 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. | |