SDO HMI 2014-09-05 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.51 | 0.00 | 8.77 | 11.57 | 177.23 | 17.51 | 291.99 | 0.3196 | -195.5 | -93.3 | |
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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 | 0.71 | 0.00 | 0.40 | 11.46 | 188.44 | 28.72 | 280.70 | 0.4812 | -687.0 | -569.5 | |
| 0.00 | 1.61 | 0.00 | 0.91 | 12.37 | 188.48 | 28.76 | 282.57 | 0.4834 | -107.0 | -136.1 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 10.88 | 186.99 | 27.26 | 279.76 | 0.4583 | -813.0 | -730.6 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 11.46 | 186.84 | 27.11 | 281.07 | 0.4570 | -729.0 | -628.8 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 11.25 | 186.40 | 26.68 | 280.70 | 0.4500 | -880.0 | -636.9 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 11.98 | 186.37 | 26.65 | 282.32 | 0.4510 | -841.0 | -648.6 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 11.57 | 185.99 | 26.26 | 281.54 | 0.4442 | -804.0 | -653.9 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 2.93 | 170.91 | 11.19 | 249.46 | 0.2078 | -765.0 | -618.7 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 15.05 | 169.21 | 9.49 | 310.88 | 0.2115 | 840.0 | 575.9 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 11.73 | 164.44 | 4.72 | 314.39 | 0.1133 | 849.0 | 589.4 | |
| 0.00 | 1.96 | 0.00 | 0.97 | 7.24 | 162.33 | 2.61 | 270.44 | 0.0454 | 741.0 | 546.3 | |
| 0.00 | 2.05 | 0.00 | 1.03 | 16.44 | 161.08 | 1.35 | 351.94 | 0.1625 | 850.0 | 807.3 | |
| 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. | |