SDO HMI 2014-03-03 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.22 | 0.00 | 10.56 | -13.10 | 74.12 | -31.00 | 103.39 | 0.5174 | -60.6 | -217.8 | |
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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 | 2.59 | 0.00 | 1.41 | -13.39 | 81.19 | -23.92 | 106.59 | 0.4134 | 795.0 | 535.6 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -14.19 | 76.73 | -28.39 | 106.39 | 0.4825 | 665.0 | 572.9 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -11.34 | 75.73 | -29.39 | 100.29 | 0.4910 | 777.0 | 668.4 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -11.19 | 75.64 | -29.48 | 99.96 | 0.4921 | 795.0 | 629.4 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -11.75 | 74.98 | -30.14 | 100.95 | 0.5027 | 544.0 | 434.5 | |
| 0.00 | 1.38 | 0.00 | 0.80 | -12.21 | 73.82 | -31.29 | 101.62 | 0.5204 | -712.0 | -638.4 | |
| 0.00 | 3.63 | 0.00 | 2.11 | -11.83 | 73.45 | -31.67 | 100.82 | 0.5253 | -765.0 | -706.0 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -11.52 | 73.34 | -31.78 | 100.22 | 0.5264 | -706.0 | -620.9 | |
| 0.00 | 1.55 | 0.00 | 0.90 | -10.89 | 73.38 | -31.73 | 99.03 | 0.5251 | -677.0 | -524.4 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -16.38 | 70.07 | -35.05 | 108.15 | 0.5820 | -730.0 | -628.8 | |
| 0.00 | 3.20 | 0.00 | 1.95 | -16.42 | 69.76 | -35.36 | 108.12 | 0.5863 | -653.0 | -539.8 | |
| 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. | |