SDO HMI 2014-01-11 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.05 | 425.80 | 48.44 | 278.63 | -16.23 | 13.78 | -39.63 | 110.19 | 0.6547 | 925.1 | 296.3 | |
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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 | 1.11 | 0.00 | 0.72 | -17.42 | 14.47 | -38.94 | 112.19 | 0.6500 | -40.0 | -26.7 | |
| 42.17 | 417.95 | 27.34 | 272.94 | -16.29 | 14.39 | -39.02 | 110.47 | 0.6473 | 1280.0 | 311.3 | |
| 2.21 | -2.00 | 1.44 | -2.00 | -16.61 | 14.00 | -39.41 | 110.81 | 0.6532 | 605.5 | 999999 | |
| 26.78 | -2.00 | 17.64 | -2.00 | -16.12 | 13.24 | -40.17 | 109.83 | 0.6612 | 1007.3 | 999999 | |
| 1.53 | -2.00 | 1.01 | -2.00 | -16.31 | 12.86 | -40.55 | 110.00 | 0.6663 | 435.2 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.86 | -16.59 | 7.36 | -46.05 | 108.91 | 0.7318 | -581.0 | -538.1 | |
| 0.00 | 0.60 | 0.00 | 0.44 | -16.73 | 6.59 | -46.82 | 108.93 | 0.7406 | -569.0 | -453.6 | |
| 0.00 | 0.60 | 0.00 | 0.43 | -14.52 | 6.76 | -46.65 | 106.00 | 0.7346 | -703.0 | -633.7 | |
| 0.00 | 1.28 | 0.00 | 0.94 | -14.50 | 6.23 | -47.18 | 105.87 | 0.7406 | -567.0 | -432.5 | |
| 1.36 | 2.30 | 1.01 | 1.71 | -15.52 | 5.57 | -47.84 | 107.11 | 0.7497 | -655.0 | -487.2 | |
| 0.00 | 0.77 | 0.00 | 0.59 | -17.31 | 4.27 | -49.14 | 109.19 | 0.7669 | -593.0 | -502.6 | |
| 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. | |