SDO HMI 2011-11-13 16:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.16 | 381.22 | 29.96 | 222.67 | 16.21 | 63.82 | 29.67 | 296.32 | 0.5326 | -785.0 | -350.6 | |
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back to the solar disc SDO HMI 2011-11-13 16:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.47 | 361.64 | 29.56 | 211.70 | 16.05 | 64.19 | 30.04 | 295.71 | 0.5361 | -1332.0 | -389.6 | |
| 0.69 | -1.00 | 0.40 | -1.00 | 16.43 | 63.65 | 29.49 | 296.73 | 0.5309 | -923.2 | 999999 | |
| 0.00 | 2.92 | 0.00 | 1.67 | 14.09 | 62.31 | 28.16 | 293.34 | 0.5005 | -916.0 | -697.4 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 15.24 | 62.47 | 28.32 | 295.38 | 0.5087 | -864.0 | -620.7 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 17.93 | 58.00 | 23.85 | 304.17 | 0.4669 | 761.0 | 572.8 | |
| 0.00 | 1.98 | 0.00 | 1.10 | 17.82 | 57.71 | 23.56 | 304.24 | 0.4623 | 827.0 | 579.9 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 18.08 | 56.84 | 22.68 | 305.67 | 0.4532 | 402.0 | 432.3 | |
| 0.00 | 1.98 | 0.00 | 1.11 | 21.20 | 55.96 | 21.81 | 312.28 | 0.4701 | 762.0 | 653.2 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 20.48 | 55.86 | 21.70 | 311.18 | 0.4622 | 520.0 | 433.9 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 21.55 | 55.44 | 21.28 | 313.52 | 0.4675 | 714.0 | 540.6 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 22.66 | 54.99 | 20.84 | 315.90 | 0.4737 | 807.0 | 632.2 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 21.54 | 54.48 | 20.33 | 314.73 | 0.4567 | 786.0 | 798.5 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 21.70 | 54.40 | 20.25 | 315.10 | 0.4575 | 836.0 | 722.8 | |
| 0.00 | 2.06 | 0.00 | 1.14 | 20.98 | 54.13 | 19.97 | 314.26 | 0.4472 | 797.0 | 628.0 | |
| 0.00 | 1.55 | 0.00 | 0.84 | 20.32 | 50.90 | 16.75 | 317.87 | 0.4047 | 724.0 | 548.3 | |
| 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. | |