SDO HMI 2014-10-12 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 | 22.59 | 0.00 | 14.90 | -22.76 | 69.01 | 29.42 | 223.69 | 0.6603 | -350.2 | -335.3 | |
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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 | 3.06 | 0.00 | 2.10 | -16.77 | 77.10 | 37.51 | 237.75 | 0.6916 | 732.0 | 575.9 | |
| 0.00 | 1.58 | 0.00 | 1.07 | -16.88 | 76.29 | 36.70 | 237.07 | 0.6837 | 471.0 | 486.6 | |
| 0.00 | 1.31 | 0.00 | 0.87 | -24.53 | 68.44 | 28.85 | 221.41 | 0.6660 | -394.0 | -333.8 | |
| 0.00 | 5.52 | 0.00 | 3.60 | -23.41 | 68.13 | 28.54 | 222.36 | 0.6531 | -887.0 | -743.8 | |
| 0.00 | 0.61 | 0.00 | 0.40 | -24.11 | 68.26 | 28.67 | 221.71 | 0.6606 | -451.0 | -433.6 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -23.65 | 68.04 | 28.45 | 222.00 | 0.6544 | -482.0 | -611.5 | |
| 0.00 | 1.23 | 0.00 | 0.84 | -26.73 | 68.84 | 29.25 | 219.46 | 0.6890 | -305.0 | -345.7 | |
| 0.00 | 2.63 | 0.00 | 1.73 | -24.20 | 68.02 | 28.43 | 221.38 | 0.6593 | -542.0 | -499.5 | |
| 0.00 | 2.01 | 0.00 | 1.32 | -24.01 | 67.79 | 28.20 | 221.36 | 0.6556 | -778.0 | -653.7 | |
| 0.00 | 1.31 | 0.00 | 0.86 | -24.13 | 67.34 | 27.75 | 220.79 | 0.6527 | -534.0 | -523.6 | |
| 0.00 | 1.14 | 0.00 | 0.71 | -26.36 | 58.26 | 18.67 | 208.34 | 0.6065 | -581.0 | -470.5 | |
| 0.00 | 1.14 | 0.00 | 0.71 | -26.54 | 58.22 | 18.63 | 208.13 | 0.6083 | -452.0 | -503.6 | |
| 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. | |