SDO HMI 2014-07-13 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.72 | 31.15 | 7.90 | 24.79 | 5.94 | 205.82 | 51.60 | 274.33 | 0.7831 | -168.5 | -242.8 | |
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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 | 0.73 | 0.00 | 0.61 | 4.28 | 208.00 | 53.78 | 272.25 | 0.8073 | 399.0 | 430.9 | |
| 1.91 | 8.17 | 1.59 | 6.84 | 5.32 | 207.91 | 53.70 | 273.55 | 0.8061 | -588.1 | -496.4 | |
| 1.82 | 11.35 | 1.48 | 9.18 | 6.03 | 206.87 | 52.66 | 274.41 | 0.7952 | -482.0 | -546.0 | |
| 5.54 | -3.00 | 4.47 | -3.00 | 6.17 | 206.54 | 52.32 | 274.58 | 0.7916 | -698.7 | 999999 | |
| 0.45 | 2.00 | 0.36 | 1.59 | 5.90 | 205.90 | 51.69 | 274.23 | 0.7848 | -644.2 | -626.4 | |
| 0.00 | 1.36 | 0.00 | 1.07 | 4.12 | 205.50 | 51.29 | 271.94 | 0.7810 | 492.0 | 292.9 | |
| 0.00 | 1.73 | 0.00 | 1.34 | 6.33 | 204.83 | 50.61 | 274.78 | 0.7731 | -577.0 | -459.5 | |
| 0.00 | 1.09 | 0.00 | 0.84 | 6.10 | 204.60 | 50.39 | 274.47 | 0.7706 | -214.0 | -323.1 | |
| 0.00 | 0.54 | 0.00 | 0.42 | 8.39 | 204.62 | 50.41 | 277.46 | 0.7711 | 363.0 | 453.3 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 9.46 | 204.78 | 50.57 | 278.84 | 0.7733 | 357.0 | 281.3 | |
| 0.00 | 0.82 | 0.00 | 0.60 | 5.63 | 202.01 | 47.79 | 273.83 | 0.7411 | 352.0 | 347.1 | |
| 0.00 | 0.64 | 0.00 | 0.46 | 8.13 | 200.98 | 46.76 | 277.26 | 0.7293 | 190.0 | 217.0 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 5.98 | 197.01 | 42.80 | 274.31 | 0.6799 | 719.0 | 646.1 | |
| 0.00 | 1.36 | 0.00 | 0.90 | 8.45 | 196.01 | 41.80 | 278.03 | 0.6681 | 383.0 | 348.5 | |
| 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. | |