SDO HMI 2014-04-13 18:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.21 | 423.43 | 37.97 | 219.76 | 11.56 | 274.80 | -0.88 | 2.81 | 0.2994 | -1019.6 | -398.1 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.69 | 13.14 | 278.07 | 2.38 | 352.87 | 0.3272 | -705.0 | -601.1 | |
| 73.21 | 403.57 | 37.97 | 209.28 | 11.46 | 275.01 | -0.67 | 2.23 | 0.2971 | -1516.3 | -434.1 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 9.53 | 273.49 | -2.20 | 8.17 | 0.2669 | -803.0 | -590.5 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 13.85 | 273.15 | -2.53 | 7.31 | 0.3392 | -892.0 | -737.7 | |
| 0.00 | 1.94 | 0.00 | 1.02 | 13.60 | 272.38 | -3.31 | 9.62 | 0.3369 | -830.0 | -635.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 7.95 | 272.31 | -3.37 | 13.85 | 0.2445 | -678.0 | -387.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.39 | 269.97 | -5.71 | 15.69 | 0.3582 | 734.0 | 553.3 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 13.18 | 269.69 | -6.00 | 17.45 | 0.3406 | 713.0 | 576.6 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 14.39 | 269.60 | -6.09 | 16.65 | 0.3600 | 777.0 | 605.6 | |
| 0.00 | 3.44 | 0.00 | 1.83 | 14.59 | 269.34 | -6.34 | 17.14 | 0.3642 | 825.0 | 676.4 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 12.52 | 269.06 | -6.63 | 19.84 | 0.3336 | 846.0 | 712.2 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 13.99 | 268.27 | -7.42 | 20.41 | 0.3607 | 779.0 | 603.2 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 13.80 | 268.21 | -7.47 | 20.75 | 0.3581 | 915.0 | 750.2 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 16.25 | 267.75 | -7.94 | 19.55 | 0.3979 | 699.0 | 558.1 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 16.78 | 267.28 | -8.40 | 20.13 | 0.4083 | 599.0 | 482.7 | |
| 0.00 | 0.53 | 0.00 | 0.28 | 13.25 | 266.70 | -8.99 | 25.13 | 0.3595 | 589.0 | 473.7 | |
| 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. | |