SDO HMI 2014-04-24 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.63 | 0.00 | 6.62 | -14.31 | 162.20 | 27.39 | 249.68 | 0.4837 | -520.7 | -453.9 | |
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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 | 0.53 | 0.00 | 0.33 | -20.47 | 169.52 | 34.71 | 241.98 | 0.6065 | -535.0 | -459.5 | |
| 0.00 | 0.80 | 0.00 | 0.52 | -28.16 | 169.84 | 35.02 | 231.00 | 0.6534 | -564.0 | -509.7 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -13.10 | 162.66 | 27.85 | 251.34 | 0.4821 | -749.0 | -549.1 | |
| 0.00 | 1.60 | 0.00 | 0.89 | -10.02 | 162.06 | 27.24 | 257.50 | 0.4636 | -730.0 | -574.7 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -17.06 | 162.80 | 27.98 | 243.71 | 0.5023 | -568.0 | -414.8 | |
| 0.00 | 2.13 | 0.00 | 1.19 | -9.89 | 161.56 | 26.75 | 257.62 | 0.4558 | -671.0 | -547.3 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -17.33 | 162.27 | 27.46 | 242.85 | 0.4967 | -713.0 | -610.1 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -9.68 | 161.34 | 26.53 | 257.99 | 0.4520 | -821.0 | -622.7 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -21.59 | 161.13 | 26.31 | 234.24 | 0.5099 | -641.0 | -470.2 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -19.75 | 159.72 | 24.91 | 236.22 | 0.4788 | -531.0 | -507.1 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -7.90 | 154.58 | 19.77 | 260.05 | 0.3416 | 795.0 | 581.7 | |
| 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. | |