SDO HMI 2014-04-26 20:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.68 | 0.00 | 11.93 | -20.30 | 139.60 | 36.72 | 242.91 | 0.6313 | 87.9 | -8.3 | |
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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 | 0.80 | 0.00 | 0.54 | -18.64 | 143.63 | 40.75 | 247.13 | 0.6736 | 456.0 | 474.9 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -18.82 | 143.13 | 40.26 | 246.69 | 0.6683 | 742.0 | 611.0 | |
| 0.00 | 2.14 | 0.00 | 1.44 | -21.00 | 143.64 | 40.76 | 243.76 | 0.6818 | 676.0 | 568.6 | |
| 0.00 | 1.51 | 0.00 | 1.00 | -19.67 | 142.46 | 39.58 | 245.21 | 0.6633 | 601.0 | 469.4 | |
| 0.00 | 0.89 | 0.00 | 0.58 | -19.36 | 141.71 | 38.83 | 245.36 | 0.6531 | 758.0 | 604.2 | |
| 0.00 | 1.07 | 0.00 | 0.69 | -20.72 | 140.83 | 37.95 | 242.97 | 0.6480 | 765.0 | 644.6 | |
| 0.00 | 0.89 | 0.00 | 0.57 | -20.60 | 140.18 | 37.30 | 242.86 | 0.6398 | 591.0 | 477.7 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -21.10 | 138.23 | 35.35 | 241.13 | 0.6187 | -572.0 | -432.9 | |
| 0.00 | 3.11 | 0.00 | 1.93 | -19.86 | 137.60 | 34.72 | 242.70 | 0.6050 | -554.0 | -446.3 | |
| 0.00 | 1.07 | 0.00 | 0.67 | -21.36 | 137.91 | 35.03 | 240.55 | 0.6161 | -580.0 | -443.5 | |
| 0.00 | 1.87 | 0.00 | 1.17 | -20.83 | 137.69 | 34.81 | 241.24 | 0.6108 | -428.0 | -395.6 | |
| 0.00 | 1.33 | 0.00 | 0.83 | -20.50 | 137.48 | 34.60 | 241.65 | 0.6067 | -653.0 | -575.2 | |
| 0.00 | 2.22 | 0.00 | 1.36 | -20.51 | 135.74 | 32.86 | 240.64 | 0.5853 | -659.0 | -495.5 | |
| 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. | |