SDO HMI 2014-05-20 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.76 | 123.95 | 41.88 | 160.50 | -11.39 | 79.25 | -67.43 | 101.49 | 0.9246 | -54.8 | -35.4 | |
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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 |
| 3.15 | 46.77 | 3.60 | 53.71 | -11.18 | 82.41 | -64.27 | 101.42 | 0.9034 | 676.6 | 287.4 | |
| 2.34 | -1.00 | 2.69 | -1.00 | -11.48 | 82.28 | -64.40 | 101.75 | 0.9045 | 393.3 | 999999 | |
| 8.01 | -1.00 | 9.18 | -1.00 | -10.80 | 82.35 | -64.33 | 101.01 | 0.9037 | 599.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 1.39 | -12.14 | 81.47 | -65.21 | 102.43 | 0.9106 | 370.0 | 290.5 | |
| 1.26 | -1.00 | 1.48 | -1.00 | -11.03 | 81.74 | -64.93 | 101.22 | 0.9082 | -89.6 | 999999 | |
| 0.00 | 1.44 | 0.00 | 1.87 | -12.90 | 79.19 | -67.48 | 103.12 | 0.9262 | 513.0 | 389.9 | |
| 1.44 | 2.79 | 1.83 | 3.55 | -11.09 | 79.64 | -67.03 | 101.18 | 0.9227 | -552.1 | -526.1 | |
| 0.00 | 2.52 | 0.00 | 3.29 | -11.19 | 79.02 | -67.65 | 101.26 | 0.9267 | -380.0 | -283.3 | |
| 0.00 | 0.54 | 0.00 | 0.75 | -13.41 | 77.52 | -69.15 | 103.57 | 0.9367 | -218.0 | -139.0 | |
| 0.00 | 0.81 | 0.00 | 1.10 | -12.37 | 78.15 | -68.53 | 102.49 | 0.9326 | 221.0 | 155.2 | |
| 1.71 | 4.14 | 2.45 | 5.93 | -13.24 | 77.01 | -69.67 | 103.36 | 0.9397 | -466.6 | -467.1 | |
| 6.75 | 62.51 | 9.20 | 87.12 | -11.28 | 77.97 | -68.71 | 101.31 | 0.9334 | -659.3 | -179.7 | |
| 0.00 | 1.26 | 0.00 | 1.79 | -12.34 | 77.11 | -69.56 | 102.41 | 0.9388 | -336.0 | -311.4 | |
| 8.10 | -12.00 | 11.45 | -12.00 | -11.54 | 77.22 | -69.46 | 101.56 | 0.9380 | -300.7 | 999999 | |
| 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. | |