SDO HMI 2011-05-05 13:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.19 | 334.08 | 24.86 | 179.87 | 17.96 | 61.01 | 7.86 | 340.56 | 0.3934 | -832.9 | -367.0 | |
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back to the solar disc SDO HMI 2011-05-05 13:59:07 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.42 | 311.65 | 23.37 | 167.75 | 17.84 | 61.27 | 8.12 | 339.88 | 0.3926 | -1377.9 | -423.0 | |
| 2.77 | -1.00 | 1.49 | -1.00 | 18.22 | 60.90 | 7.75 | 341.06 | 0.3965 | -1000.9 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.92 | 19.37 | 60.67 | 7.52 | 342.52 | 0.4126 | -783.0 | -467.1 | |
| 0.00 | 1.88 | 0.00 | 1.06 | 24.22 | 60.03 | 6.88 | 346.88 | 0.4830 | -878.0 | -649.1 | |
| 0.00 | 1.25 | 0.00 | 0.68 | 19.42 | 59.51 | 6.36 | 345.12 | 0.4083 | -718.0 | -549.8 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 19.19 | 59.27 | 6.12 | 345.49 | 0.4038 | -701.0 | -497.8 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 17.42 | 57.94 | 4.79 | 347.56 | 0.3710 | 847.0 | 634.2 | |
| 0.00 | 6.52 | 0.00 | 3.48 | 17.78 | 57.82 | 4.67 | 348.06 | 0.3762 | 647.0 | 604.1 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 17.84 | 57.57 | 4.41 | 348.73 | 0.3764 | 836.0 | 655.9 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 18.46 | 57.49 | 4.33 | 349.25 | 0.3860 | 929.0 | 742.9 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 19.04 | 56.38 | 3.23 | 352.17 | 0.3924 | 693.0 | 647.2 | |
| 0.00 | 1.70 | 0.00 | 0.95 | 23.72 | 55.69 | 2.54 | 354.97 | 0.4647 | 652.0 | 512.7 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 18.84 | 55.48 | 2.33 | 354.28 | 0.3875 | 780.0 | 497.5 | |
| 0.00 | 1.52 | 0.00 | 0.82 | 19.66 | 54.37 | 1.22 | 357.12 | 0.3993 | 689.0 | 500.0 | |
| 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. | |