SDO HMI 2014-09-12 17:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.95 | 24.56 | 1.44 | 18.24 | -20.22 | 106.33 | 40.15 | 234.29 | 0.7464 | 210.9 | 263.8 | |
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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 |
| 0.00 | 1.51 | 0.00 | 1.18 | -19.42 | 110.04 | 43.86 | 237.55 | 0.7766 | 68.0 | 128.6 | |
| 0.00 | 5.07 | 0.00 | 4.00 | -20.00 | 110.15 | 43.97 | 236.95 | 0.7806 | 538.0 | 430.4 | |
| 0.00 | 0.80 | 0.00 | 0.62 | -21.43 | 108.44 | 42.26 | 234.34 | 0.7727 | 399.0 | 372.2 | |
| 0.00 | 1.16 | 0.00 | 0.87 | -20.71 | 107.24 | 41.06 | 234.42 | 0.7577 | 640.0 | 551.5 | |
| 0.00 | 2.76 | 0.00 | 2.07 | -20.33 | 107.07 | 40.89 | 234.75 | 0.7539 | 716.0 | 588.3 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -21.43 | 106.96 | 40.78 | 233.42 | 0.7594 | 447.0 | 509.7 | |
| 0.62 | 1.51 | 0.46 | 1.11 | -19.73 | 105.99 | 39.82 | 234.76 | 0.7403 | 709.4 | 580.1 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -19.06 | 105.63 | 39.45 | 235.30 | 0.7328 | 569.0 | 508.9 | |
| 0.00 | 1.07 | 0.00 | 0.77 | -19.01 | 105.37 | 39.19 | 235.20 | 0.7299 | 568.0 | 547.5 | |
| 1.33 | 3.47 | 0.98 | 2.55 | -20.46 | 105.55 | 39.37 | 233.61 | 0.7405 | 712.4 | 574.2 | |
| 0.00 | 1.16 | 0.00 | 0.85 | -20.51 | 105.31 | 39.13 | 233.40 | 0.7386 | 676.0 | 492.6 | |
| 0.00 | 0.98 | 0.00 | 0.67 | -18.12 | 102.32 | 36.14 | 234.14 | 0.6939 | -567.0 | -474.6 | |
| 0.00 | 0.71 | 0.00 | 0.49 | -18.73 | 102.03 | 35.85 | 233.19 | 0.6951 | -523.0 | -524.1 | |
| 0.00 | 0.62 | 0.00 | 0.43 | -18.45 | 101.80 | 35.63 | 233.36 | 0.6909 | -464.0 | -411.1 | |
| 0.00 | 0.89 | 0.00 | 0.61 | -18.74 | 101.72 | 35.54 | 232.94 | 0.6921 | -692.0 | -488.6 | |
| 0.00 | 1.96 | 0.00 | 1.37 | -23.94 | 99.29 | 33.11 | 225.02 | 0.7081 | -641.0 | -568.0 | |
| 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. | |