SDO HMI 2014-10-10 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.45 | 0.00 | 8.76 | 13.01 | 61.41 | -4.56 | 266.25 | 0.1546 | -286.9 | -168.9 | |
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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 | 0.88 | 0.00 | 0.44 | 11.01 | 69.96 | 3.98 | 320.72 | 0.1082 | -726.0 | -528.7 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.43 | 67.42 | 1.44 | 350.28 | 0.1452 | -771.0 | -551.6 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 13.17 | 65.66 | -0.32 | 2.56 | 0.1212 | -775.0 | -586.8 | |
| 0.00 | 1.05 | 0.00 | 0.52 | 11.69 | 65.05 | -0.93 | 9.49 | 0.0968 | -798.0 | -563.4 | |
| 0.00 | 1.40 | 0.00 | 0.71 | 15.86 | 63.29 | -2.68 | 15.08 | 0.1739 | -789.0 | -635.8 | |
| 0.00 | 1.49 | 0.00 | 0.74 | 10.94 | 63.22 | -2.76 | 29.95 | 0.0950 | -680.0 | -472.2 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 10.52 | 62.92 | -3.06 | 35.09 | 0.0917 | -986.0 | -770.4 | |
| 0.00 | 2.72 | 0.00 | 1.35 | 10.64 | 62.52 | -3.46 | 37.66 | 0.0974 | -876.0 | -680.0 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 18.87 | 61.10 | -4.88 | 20.19 | 0.2343 | -815.0 | -593.7 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 12.69 | 59.45 | -6.53 | 44.50 | 0.1590 | 887.0 | 637.5 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 13.47 | 57.25 | -8.72 | 49.26 | 0.1955 | 999.0 | 796.0 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 13.71 | 55.24 | -10.73 | 53.93 | 0.2248 | 811.0 | 545.7 | |
| 0.00 | 1.67 | 0.00 | 0.85 | 13.85 | 53.41 | -12.56 | 57.42 | 0.2518 | 789.0 | 673.5 | |
| 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. | |