SDO HMI 2014-09-25 14:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.21 | 23.85 | 1.67 | 17.95 | 7.03 | 207.07 | -49.16 | 86.74 | 0.7541 | -122.9 | 39.3 | |
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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 | 1.15 | 0.00 | 0.83 | 6.67 | 209.30 | -46.93 | 87.37 | 0.7286 | -508.0 | -438.2 | |
| 0.00 | 1.94 | 0.00 | 1.40 | 7.17 | 209.15 | -47.08 | 86.67 | 0.7301 | -703.0 | -523.2 | |
| 0.00 | 0.62 | 0.00 | 0.45 | 6.96 | 209.17 | -47.05 | 86.96 | 0.7299 | -596.0 | -500.7 | |
| 0.00 | 1.50 | 0.00 | 1.09 | 6.35 | 209.07 | -47.16 | 87.79 | 0.7316 | -673.0 | -591.4 | |
| 0.00 | 0.97 | 0.00 | 0.71 | 6.49 | 208.92 | -47.31 | 87.59 | 0.7333 | -526.0 | -468.2 | |
| 0.88 | 2.21 | 0.64 | 1.61 | 6.11 | 208.79 | -47.44 | 88.09 | 0.7351 | -495.1 | -408.3 | |
| 0.00 | 1.59 | 0.00 | 1.16 | 6.31 | 208.67 | -47.56 | 87.81 | 0.7363 | -355.0 | -260.9 | |
| 0.00 | 1.24 | 0.00 | 0.91 | 7.17 | 208.15 | -48.07 | 86.60 | 0.7418 | -681.0 | -512.0 | |
| 0.00 | 0.97 | 0.00 | 0.72 | 7.37 | 207.94 | -48.28 | 86.33 | 0.7441 | -430.0 | -349.0 | |
| 0.00 | 1.94 | 0.00 | 1.49 | 6.89 | 206.01 | -50.22 | 86.83 | 0.7664 | 813.0 | 711.9 | |
| 0.00 | 0.62 | 0.00 | 0.48 | 5.98 | 206.03 | -50.20 | 88.01 | 0.7668 | 314.0 | 341.0 | |
| 1.33 | 5.30 | 1.03 | 4.11 | 7.00 | 205.51 | -50.72 | 86.65 | 0.7718 | 635.0 | 614.7 | |
| 0.00 | 0.62 | 0.00 | 0.48 | 6.94 | 205.28 | -50.95 | 86.70 | 0.7744 | 277.0 | 275.3 | |
| 0.00 | 1.77 | 0.00 | 1.39 | 8.56 | 204.72 | -51.51 | 84.59 | 0.7798 | 560.0 | 543.2 | |
| 0.00 | 1.41 | 0.00 | 1.12 | 8.72 | 204.49 | -51.74 | 84.37 | 0.7822 | 368.0 | 304.1 | |
| 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. | |