SDO HMI 2014-08-01 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.31 | 0.00 | 10.25 | 11.05 | 258.56 | -6.49 | 178.18 | 0.1782 | 451.3 | 296.0 | |
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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 | 1.63 | 0.00 | 0.82 | 16.13 | 267.49 | 2.43 | 347.21 | 0.1849 | -876.0 | -643.2 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 15.70 | 267.13 | 2.08 | 348.54 | 0.1764 | -887.0 | -744.4 | |
| 0.00 | 2.45 | 0.00 | 1.22 | 12.32 | 263.67 | -1.38 | 11.72 | 0.1167 | -795.0 | -685.7 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 1.25 | 260.76 | -4.29 | 136.55 | 0.1093 | 837.0 | 660.5 | |
| 0.00 | 1.99 | 0.00 | 0.99 | 9.71 | 260.37 | -4.68 | 49.53 | 0.1063 | 1039.0 | 841.1 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 7.39 | 259.94 | -5.12 | 72.26 | 0.0933 | 874.0 | 787.6 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 8.63 | 258.78 | -6.28 | 65.13 | 0.1197 | 736.0 | 521.2 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 16.17 | 258.47 | -6.58 | 31.34 | 0.2126 | 698.0 | 637.5 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 14.24 | 256.95 | -8.10 | 42.75 | 0.2022 | 779.0 | 577.2 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 4.37 | 255.96 | -9.09 | 98.53 | 0.1601 | 1011.0 | 838.0 | |
| 0.00 | 2.54 | 0.00 | 1.27 | 4.67 | 255.74 | -9.31 | 96.48 | 0.1631 | 929.0 | 739.2 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 15.27 | 249.62 | -15.43 | 56.76 | 0.3082 | 636.0 | 501.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 14.20 | 248.69 | -16.37 | 61.20 | 0.3131 | 799.0 | 500.0 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 16.18 | 244.66 | -20.40 | 60.89 | 0.3848 | 538.0 | 315.3 | |
| 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. | |