SDO HMI 2014-03-29 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.82 | 0.00 | 10.66 | -27.91 | 84.37 | -33.11 | 129.02 | 0.6115 | 51.2 | 34.6 | |
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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 | 0.88 | 0.00 | 0.47 | -22.78 | 101.78 | -15.71 | 138.44 | 0.3778 | 820.0 | 697.6 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -20.62 | 97.79 | -19.69 | 128.12 | 0.4026 | 698.0 | 554.9 | |
| 0.00 | 1.66 | 0.00 | 0.95 | -25.81 | 94.28 | -23.21 | 133.47 | 0.4908 | 803.0 | 688.2 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -26.90 | 90.96 | -26.52 | 131.85 | 0.5367 | 723.0 | 576.3 | |
| 0.00 | 2.02 | 0.00 | 1.19 | -27.02 | 90.18 | -27.30 | 131.32 | 0.5463 | 902.0 | 711.3 | |
| 0.00 | 1.75 | 0.00 | 1.04 | -27.01 | 89.88 | -27.60 | 131.03 | 0.5494 | 705.0 | 613.5 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -27.28 | 82.29 | -35.19 | 125.90 | 0.6347 | -646.0 | -479.4 | |
| 0.00 | 1.31 | 0.00 | 0.85 | -27.58 | 81.97 | -35.51 | 126.14 | 0.6399 | -566.0 | -405.3 | |
| 0.00 | 2.10 | 0.00 | 1.41 | -29.88 | 79.65 | -37.83 | 127.99 | 0.6770 | -455.0 | -381.3 | |
| 0.00 | 1.66 | 0.00 | 1.22 | -33.89 | 75.33 | -42.15 | 130.88 | 0.7392 | -581.0 | -347.6 | |
| 0.00 | 0.53 | 0.00 | 0.39 | -34.07 | 75.07 | -42.41 | 130.99 | 0.7424 | -492.0 | -432.0 | |
| 0.00 | 1.23 | 0.00 | 0.85 | -26.56 | 75.65 | -41.83 | 121.57 | 0.7026 | -694.0 | -541.0 | |
| 0.00 | 1.14 | 0.00 | 0.79 | -26.73 | 75.39 | -42.09 | 121.70 | 0.7060 | -552.0 | -537.6 | |
| 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. | |