SDO HMI 2014-05-20 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.56 | 22.59 | 8.42 | 25.77 | -18.02 | 217.37 | 63.55 | 250.97 | 0.9022 | -61.4 | 119.6 | |
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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 |
| 0.90 | 1.98 | 1.11 | 2.44 | -18.63 | 219.50 | 65.68 | 250.55 | 0.9175 | 329.5 | 298.8 | |
| 0.00 | 3.60 | 0.00 | 4.25 | -17.71 | 218.38 | 64.56 | 251.43 | 0.9093 | 512.0 | 283.2 | |
| 0.00 | 1.26 | 0.00 | 1.49 | -18.02 | 218.45 | 64.62 | 251.09 | 0.9100 | 241.0 | 184.2 | |
| 0.00 | 2.25 | 0.00 | 2.70 | -18.71 | 218.79 | 64.96 | 250.37 | 0.9128 | 25.0 | 79.2 | |
| 0.00 | 0.54 | 0.00 | 0.63 | -17.41 | 217.89 | 64.06 | 251.70 | 0.9056 | 507.0 | 443.2 | |
| 0.00 | 1.44 | 0.00 | 1.69 | -18.19 | 218.12 | 64.29 | 250.86 | 0.9078 | 544.0 | 447.3 | |
| 0.00 | 0.27 | 0.00 | 0.31 | -17.84 | 217.15 | 63.33 | 251.14 | 0.9007 | 502.0 | 553.7 | |
| 0.00 | 1.35 | 0.00 | 1.43 | -15.43 | 215.49 | 61.66 | 253.63 | 0.8862 | -324.0 | -282.3 | |
| 6.66 | 8.73 | 7.31 | 9.58 | -18.22 | 216.19 | 62.37 | 250.60 | 0.8941 | -380.9 | -194.2 | |
| 0.00 | 0.90 | 0.00 | 0.95 | -17.46 | 215.12 | 61.30 | 251.30 | 0.8852 | -251.0 | -270.1 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -19.34 | 216.16 | 62.33 | 249.35 | 0.8949 | -406.0 | -385.7 | |
| 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. | |