SDO HMI 2014-04-05 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.40 | 0.00 | 7.82 | 5.40 | 24.75 | 1.27 | 351.06 | 0.2172 | -19.7 | -53.6 | |
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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 | 2.11 | 0.00 | 1.07 | 3.38 | 28.93 | 5.45 | 330.48 | 0.1932 | -808.0 | -663.2 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 5.79 | 28.14 | 4.65 | 338.87 | 0.2248 | -741.0 | -570.6 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 1.46 | 28.05 | 4.56 | 329.39 | 0.1569 | -917.0 | -697.9 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 3.65 | 28.03 | 4.54 | 335.33 | 0.1902 | -734.0 | -543.7 | |
| 0.00 | 1.93 | 0.00 | 0.97 | 1.91 | 27.57 | 4.08 | 333.42 | 0.1598 | -883.0 | -647.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 4.13 | 26.29 | 2.80 | 344.90 | 0.1878 | -879.0 | -768.5 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 9.95 | 24.68 | 1.20 | 355.79 | 0.2814 | 816.0 | 592.0 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 8.08 | 24.46 | 0.98 | 356.11 | 0.2497 | 687.0 | 563.4 | |
| 0.00 | 1.67 | 0.00 | 0.86 | 8.68 | 21.64 | -1.84 | 7.02 | 0.2611 | 723.0 | 672.9 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 7.52 | 19.13 | -4.35 | 17.53 | 0.2509 | 729.0 | 574.6 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 5.11 | 17.55 | -5.94 | 27.62 | 0.2232 | 924.0 | 715.2 | |
| 0.00 | 1.41 | 0.00 | 0.72 | 7.14 | 17.01 | -6.47 | 25.80 | 0.2582 | 847.0 | 691.2 | |
| 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. | |