SDO HMI 2014-04-13 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.52 | 431.97 | 35.20 | 225.44 | 11.44 | 274.75 | -6.43 | 20.33 | 0.3161 | -1047.8 | -389.7 | |
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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 | 13.30 | 275.05 | -6.13 | 17.69 | 0.3434 | -775.0 | -599.1 | |
| 67.52 | 414.12 | 35.20 | 215.88 | 11.34 | 274.94 | -6.24 | 19.97 | 0.3133 | -1511.9 | -417.3 | |
| 0.00 | 2.39 | 0.00 | 1.27 | 13.74 | 272.86 | -8.32 | 22.92 | 0.3627 | -789.0 | -633.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 13.93 | 272.76 | -8.42 | 22.95 | 0.3662 | -626.0 | -492.0 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 12.89 | 272.33 | -8.86 | 25.23 | 0.3535 | -837.0 | -632.5 | |
| 0.00 | 2.03 | 0.00 | 1.06 | 9.10 | 271.73 | -9.45 | 32.46 | 0.3035 | -847.0 | -614.0 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 14.96 | 269.65 | -11.53 | 28.77 | 0.4028 | 748.0 | 633.9 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 15.76 | 269.51 | -11.67 | 28.09 | 0.4151 | 772.0 | 661.3 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 14.48 | 269.46 | -11.72 | 29.79 | 0.3977 | 900.0 | 813.3 | |
| 0.00 | 1.59 | 0.00 | 0.86 | 14.64 | 269.42 | -11.76 | 29.67 | 0.4003 | 935.0 | 693.2 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 12.89 | 269.10 | -12.09 | 32.74 | 0.3790 | 849.0 | 595.1 | |
| 0.00 | 0.71 | 0.00 | 0.38 | 14.18 | 268.36 | -12.82 | 32.44 | 0.4028 | 800.0 | 647.6 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 14.29 | 268.13 | -13.05 | 32.76 | 0.4061 | 901.0 | 690.2 | |
| 0.00 | 2.30 | 0.00 | 1.25 | 14.90 | 267.94 | -13.24 | 32.31 | 0.4159 | 684.0 | 600.6 | |
| 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. | |