SDO HMI 2014-01-10 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.89 | 0.00 | 11.43 | -17.41 | 69.29 | 8.20 | 205.48 | 0.3052 | -129.9 | -23.8 | |
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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 | 2.12 | 0.00 | 1.13 | -12.86 | 81.50 | 20.41 | 245.22 | 0.3761 | -731.0 | -620.5 | |
| 0.00 | 2.80 | 0.00 | 1.48 | -16.71 | 76.88 | 15.79 | 229.69 | 0.3433 | 910.0 | 757.7 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -18.43 | 75.55 | 14.46 | 223.48 | 0.3459 | 782.0 | 602.6 | |
| 0.00 | 2.89 | 0.00 | 1.52 | -17.95 | 75.06 | 13.98 | 223.55 | 0.3349 | 884.0 | 800.1 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -18.44 | 74.91 | 13.82 | 222.21 | 0.3389 | 845.0 | 705.5 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -19.76 | 74.41 | 13.32 | 218.57 | 0.3494 | 833.0 | 680.5 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -13.31 | 73.47 | 12.39 | 232.20 | 0.2654 | -814.0 | -677.0 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -22.07 | 71.89 | 10.80 | 209.25 | 0.3569 | 824.0 | 671.8 | |
| 0.00 | 1.70 | 0.00 | 0.86 | -16.48 | 63.60 | 2.51 | 191.09 | 0.2197 | -948.0 | -726.0 | |
| 0.00 | 2.29 | 0.00 | 1.16 | -16.23 | 59.67 | -1.42 | 173.56 | 0.2128 | -987.0 | -792.9 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -18.96 | 58.62 | -2.47 | 170.97 | 0.2611 | -845.0 | -638.0 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -17.38 | 58.27 | -2.82 | 168.47 | 0.2358 | -789.0 | -637.9 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -16.02 | 54.60 | -6.49 | 152.35 | 0.2351 | -932.0 | -678.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -25.18 | 52.74 | -8.35 | 159.97 | 0.3854 | -851.0 | -761.2 | |
| 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. | |