SDO HMI 2014-07-03 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.80 | 49.75 | 14.94 | 40.91 | -15.85 | 233.32 | -49.91 | 112.64 | 0.7986 | -23.0 | 180.4 | |
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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 |
| 0.00 | 0.82 | 0.00 | 0.59 | -15.88 | 239.78 | -43.46 | 115.22 | 0.7335 | 551.0 | 458.9 | |
| 0.00 | 2.18 | 0.00 | 1.58 | -15.46 | 239.85 | -43.39 | 114.71 | 0.7311 | 735.0 | 502.8 | |
| 1.00 | 15.34 | 0.78 | 11.94 | -14.58 | 235.57 | -47.67 | 111.86 | 0.7732 | 659.9 | 530.2 | |
| 3.54 | -3.00 | 2.75 | -3.00 | -14.26 | 235.61 | -47.62 | 111.48 | 0.7717 | 854.8 | 999999 | |
| 2.18 | -3.00 | 1.70 | -3.00 | -14.46 | 235.32 | -47.92 | 111.63 | 0.7753 | 528.6 | 999999 | |
| 0.00 | 4.27 | 0.00 | 3.36 | -14.73 | 234.95 | -48.28 | 111.83 | 0.7799 | 465.0 | 163.6 | |
| 0.00 | 0.91 | 0.00 | 0.72 | -15.38 | 234.71 | -48.53 | 112.54 | 0.7844 | 449.0 | 369.2 | |
| 0.00 | 2.63 | 0.00 | 2.13 | -16.11 | 234.08 | -49.15 | 113.21 | 0.7930 | 566.0 | 377.2 | |
| 0.00 | 0.91 | 0.00 | 0.73 | -15.44 | 234.11 | -49.13 | 112.40 | 0.7906 | -186.0 | -153.1 | |
| 0.00 | 1.54 | 0.00 | 1.27 | -15.99 | 233.24 | -50.00 | 112.76 | 0.8008 | -420.0 | -420.2 | |
| 11.08 | 21.15 | 9.71 | 18.59 | -17.03 | 230.70 | -52.53 | 113.14 | 0.8275 | -662.0 | -102.6 | |
| 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. | |