SDO HMI 2014-05-14 06:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.32 | 252.46 | 26.43 | 170.89 | -23.81 | 193.95 | -38.69 | 122.84 | 0.6824 | 620.3 | 293.1 | |
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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 |
| 1.35 | 242.29 | 0.90 | 163.01 | -23.86 | 194.84 | -37.80 | 123.37 | 0.6735 | 1067.0 | 337.1 | |
| 37.97 | -1.00 | 25.53 | -1.00 | -23.68 | 194.31 | -38.33 | 122.84 | 0.6782 | 1013.8 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.58 | -23.36 | 189.21 | -43.43 | 119.97 | 0.7308 | -485.0 | -423.9 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -25.95 | 187.72 | -44.92 | 122.62 | 0.7561 | -527.0 | -485.7 | |
| 0.00 | 0.90 | 0.00 | 0.68 | -25.81 | 187.46 | -45.18 | 122.33 | 0.7580 | -607.0 | -540.4 | |
| 0.00 | 1.80 | 0.00 | 1.38 | -26.38 | 186.73 | -45.91 | 122.74 | 0.7672 | -627.0 | -551.8 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -26.39 | 185.89 | -46.75 | 122.41 | 0.7751 | -519.0 | -449.4 | |
| 0.00 | 1.89 | 0.00 | 1.48 | -26.35 | 185.71 | -46.92 | 122.30 | 0.7766 | -538.0 | -464.7 | |
| 0.00 | 1.35 | 0.00 | 1.05 | -26.02 | 185.79 | -46.85 | 121.92 | 0.7747 | -506.0 | -367.2 | |
| 0.00 | 1.62 | 0.00 | 1.31 | -27.85 | 184.61 | -48.03 | 123.69 | 0.7922 | -656.0 | -509.2 | |
| 0.00 | 0.72 | 0.00 | 0.57 | -26.49 | 185.09 | -47.55 | 122.23 | 0.7830 | -400.0 | -364.1 | |
| 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. | |