SDO HMI 2014-03-24 10:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.36 | 39.67 | 8.29 | 29.10 | 3.31 | 137.52 | -46.45 | 79.04 | 0.7392 | 87.1 | -26.8 | |
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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 |
| 1.14 | 8.91 | 0.81 | 6.38 | 3.40 | 138.89 | -45.08 | 78.53 | 0.7236 | -596.9 | -387.5 | |
| 2.18 | -1.00 | 1.56 | -1.00 | 3.16 | 138.82 | -45.15 | 78.87 | 0.7238 | -566.3 | 999999 | |
| 0.00 | 1.75 | 0.00 | 1.26 | 3.84 | 138.35 | -45.62 | 78.10 | 0.7311 | -705.0 | -598.8 | |
| 3.23 | 8.13 | 2.35 | 5.93 | 3.93 | 138.04 | -45.93 | 78.08 | 0.7349 | -656.9 | -387.2 | |
| 0.00 | 1.22 | 0.00 | 0.89 | 3.22 | 137.87 | -46.10 | 79.08 | 0.7350 | 609.0 | 518.1 | |
| 0.00 | 1.75 | 0.00 | 1.28 | 3.71 | 137.80 | -46.17 | 78.45 | 0.7371 | 469.0 | 390.1 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 3.56 | 137.81 | -46.16 | 78.65 | 0.7366 | 373.0 | 375.8 | |
| 0.00 | 0.79 | 0.00 | 0.57 | 3.41 | 137.77 | -46.20 | 78.86 | 0.7366 | 557.0 | 478.2 | |
| 0.00 | 0.79 | 0.00 | 0.58 | 3.45 | 137.59 | -46.38 | 78.85 | 0.7388 | 346.0 | 402.2 | |
| 1.66 | 4.89 | 1.23 | 3.63 | 3.85 | 136.86 | -47.10 | 78.54 | 0.7481 | -450.7 | -353.1 | |
| 0.00 | 1.75 | 0.00 | 1.30 | 3.13 | 136.51 | -47.46 | 79.59 | 0.7503 | 244.0 | 191.4 | |
| 3.15 | 5.50 | 2.34 | 4.10 | 2.31 | 136.51 | -47.46 | 80.66 | 0.7484 | 645.6 | 485.6 | |
| 0.00 | 0.35 | 0.00 | 0.27 | 2.52 | 135.47 | -48.50 | 80.65 | 0.7606 | 530.0 | 513.8 | |
| 0.00 | 2.18 | 0.00 | 1.67 | 2.37 | 135.20 | -48.77 | 80.92 | 0.7632 | 607.0 | 483.4 | |
| 0.00 | 0.70 | 0.00 | 0.54 | 2.53 | 135.06 | -48.91 | 80.75 | 0.7652 | 517.0 | 390.1 | |
| 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. | |