SDO HMI 2014-04-03 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.88 | 58.15 | 11.63 | 35.71 | -8.49 | 8.94 | -36.52 | 95.64 | 0.5934 | 492.3 | 416.2 | |
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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 | 1.14 | 0.00 | 0.68 | -4.33 | 11.15 | -34.31 | 88.29 | 0.5645 | 697.0 | 527.9 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -8.71 | 10.47 | -34.99 | 96.06 | 0.5722 | 450.0 | 345.9 | |
| 8.43 | 12.30 | 5.09 | 7.43 | -8.36 | 10.28 | -35.18 | 95.45 | 0.5748 | 932.6 | 557.4 | |
| 4.13 | 30.66 | 2.51 | 18.65 | -8.57 | 9.77 | -35.69 | 95.80 | 0.5820 | 978.9 | 513.1 | |
| 2.72 | -4.00 | 1.66 | -4.00 | -8.76 | 9.42 | -36.05 | 96.11 | 0.5871 | 775.1 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -8.65 | 8.64 | -36.83 | 95.89 | 0.5980 | 552.0 | 461.0 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -8.26 | 8.64 | -36.82 | 95.24 | 0.5978 | 689.0 | 521.0 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -7.51 | 8.72 | -36.74 | 93.98 | 0.5967 | 575.0 | 482.2 | |
| 0.00 | 1.41 | 0.00 | 0.87 | -8.85 | 8.46 | -37.00 | 96.22 | 0.6004 | 267.0 | 302.6 | |
| 0.00 | 1.23 | 0.00 | 0.79 | -12.76 | 5.67 | -39.79 | 102.29 | 0.6411 | 119.0 | 180.2 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -12.17 | 5.42 | -40.04 | 101.33 | 0.6437 | 618.0 | 552.0 | |
| 3.60 | 5.62 | 2.37 | 3.70 | -7.57 | 4.02 | -41.44 | 94.19 | 0.6601 | -811.6 | -635.7 | |
| 0.00 | 0.53 | 0.00 | 0.35 | -7.20 | 3.17 | -42.29 | 93.66 | 0.6713 | -378.0 | -393.2 | |
| 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. | |