SDO HMI 2014-05-16 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.25 | 25.79 | 9.06 | 25.02 | -18.26 | 143.41 | -58.39 | 109.84 | 0.8607 | 352.0 | 161.0 | |
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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 | 0.81 | 0.00 | 0.60 | -17.98 | 155.34 | -46.46 | 112.08 | 0.7463 | 209.0 | 232.9 | |
| 0.00 | 0.54 | 0.00 | 0.46 | -16.56 | 147.84 | -53.96 | 108.55 | 0.8197 | 200.0 | 228.2 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -19.01 | 146.39 | -55.41 | 111.21 | 0.8370 | 511.0 | 446.7 | |
| 0.00 | 0.90 | 0.00 | 0.83 | -18.41 | 145.43 | -56.37 | 110.32 | 0.8445 | 562.0 | 497.0 | |
| 0.00 | 1.26 | 0.00 | 1.16 | -18.27 | 145.21 | -56.59 | 110.12 | 0.8463 | 573.0 | 470.1 | |
| 0.00 | 1.80 | 0.00 | 1.69 | -18.50 | 144.56 | -57.24 | 110.28 | 0.8522 | 325.0 | 232.6 | |
| 0.00 | 2.25 | 0.00 | 2.11 | -18.22 | 144.59 | -57.21 | 109.95 | 0.8516 | 281.0 | 276.0 | |
| 9.25 | 12.84 | 9.06 | 12.58 | -18.29 | 143.03 | -58.77 | 109.78 | 0.8648 | 526.2 | 341.5 | |
| 0.00 | 3.14 | 0.00 | 3.12 | -18.18 | 142.53 | -59.26 | 109.57 | 0.8687 | -292.0 | -231.3 | |
| 0.00 | 1.17 | 0.00 | 1.37 | -18.07 | 137.27 | -64.53 | 108.79 | 0.9084 | -221.0 | -246.5 | |
| 0.00 | 0.27 | 0.00 | 0.37 | -18.40 | 133.54 | -68.25 | 108.80 | 0.9326 | -206.0 | -204.0 | |
| 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. | |