SDO HMI 2014-02-25 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.50 | 133.86 | 28.52 | 107.23 | 8.26 | 132.49 | -49.47 | 73.49 | 0.7864 | 437.6 | 164.9 | |
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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 | 1.55 | 0.00 | 1.04 | 7.25 | 142.20 | -39.76 | 70.86 | 0.6740 | -684.0 | -675.1 | |
| 0.00 | 0.86 | 0.00 | 0.59 | 7.37 | 140.32 | -41.64 | 71.56 | 0.6970 | -466.0 | -385.0 | |
| 0.00 | 0.86 | 0.00 | 0.60 | 7.98 | 140.09 | -41.87 | 70.85 | 0.7021 | -644.0 | -571.8 | |
| 0.00 | 1.46 | 0.00 | 1.03 | 8.84 | 139.32 | -42.64 | 70.04 | 0.7145 | -683.0 | -561.2 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 9.62 | 139.16 | -42.80 | 69.08 | 0.7195 | -471.0 | -327.2 | |
| 0.00 | 0.95 | 0.00 | 0.67 | 7.32 | 138.78 | -43.18 | 72.30 | 0.7148 | -510.0 | -420.7 | |
| 0.00 | 0.52 | 0.00 | 0.39 | 7.62 | 134.86 | -47.10 | 73.45 | 0.7598 | 475.0 | 430.8 | |
| 2.15 | 6.89 | 1.63 | 5.23 | 7.23 | 134.78 | -47.18 | 73.98 | 0.7594 | -527.0 | -390.9 | |
| 1.21 | -8.00 | 0.92 | -8.00 | 7.13 | 134.62 | -47.34 | 74.17 | 0.7608 | -673.5 | 999999 | |
| 0.95 | 5.69 | 0.75 | 4.49 | 6.85 | 132.76 | -49.20 | 75.16 | 0.7798 | -361.3 | 50.0 | |
| 7.24 | 109.40 | 5.82 | 88.71 | 8.82 | 132.35 | -49.61 | 72.88 | 0.7898 | 982.5 | 227.8 | |
| 0.00 | 1.46 | 0.00 | 1.17 | 7.59 | 132.38 | -49.59 | 74.37 | 0.7860 | 579.0 | 542.6 | |
| 0.00 | 1.55 | 0.00 | 1.24 | 7.68 | 132.08 | -49.88 | 74.36 | 0.7892 | 517.0 | 472.6 | |
| 23.95 | -11.00 | 19.40 | -11.00 | 8.28 | 131.84 | -50.12 | 73.70 | 0.7935 | 743.8 | 999999 | |
| 0.00 | 1.64 | 0.00 | 1.34 | 9.10 | 131.64 | -50.32 | 72.78 | 0.7978 | 344.0 | 267.7 | |
| 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. | |