SDO HMI 2014-05-29 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.78 | 41.14 | 9.20 | 23.62 | -19.64 | 51.14 | 24.10 | 229.59 | 0.5054 | 290.2 | 51.2 | |
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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 | 1.08 | 0.00 | 0.64 | -20.07 | 54.77 | 27.72 | 233.02 | 0.5491 | 521.0 | 400.3 | |
| 12.45 | 17.42 | 7.30 | 10.20 | -19.47 | 54.07 | 27.03 | 233.33 | 0.5362 | 897.1 | 627.5 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -18.70 | 53.83 | 26.79 | 234.35 | 0.5274 | 690.0 | 571.3 | |
| 0.90 | 2.08 | 0.53 | 1.21 | -19.37 | 53.70 | 26.65 | 233.13 | 0.5310 | 962.8 | 871.4 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -18.92 | 53.37 | 26.32 | 233.54 | 0.5236 | 655.0 | 633.3 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -19.44 | 52.35 | 25.30 | 231.69 | 0.5156 | 675.0 | 466.5 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -19.80 | 50.74 | 23.69 | 229.38 | 0.5000 | -755.0 | -625.2 | |
| 0.00 | 2.08 | 0.00 | 1.16 | -16.43 | 50.05 | 23.01 | 234.45 | 0.4627 | 826.0 | 645.5 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -20.55 | 50.54 | 23.49 | 227.97 | 0.5045 | 735.0 | 651.0 | |
| 1.08 | 2.62 | 0.61 | 1.47 | -19.56 | 48.74 | 21.69 | 227.44 | 0.4748 | -990.1 | -826.9 | |
| 1.35 | 3.52 | 0.76 | 1.98 | -19.88 | 48.54 | 21.50 | 226.66 | 0.4757 | -898.3 | -758.3 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -19.79 | 46.02 | 18.97 | 223.39 | 0.4470 | -824.0 | -660.4 | |
| 0.00 | 2.44 | 0.00 | 1.34 | -21.87 | 42.65 | 15.60 | 214.93 | 0.4377 | -825.0 | -529.1 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -21.84 | 42.31 | 15.26 | 214.40 | 0.4342 | -807.0 | -672.3 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -21.56 | 38.45 | 11.40 | 207.58 | 0.3988 | -802.0 | -689.3 | |
| 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. | |