SDO HMI 2014-09-13 04:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 16.57 | 0.29 | 13.29 | -19.99 | 104.95 | 44.84 | 237.36 | 0.7880 | -91.9 | 4.2 | |
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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 | 1.34 | 0.00 | 1.19 | -19.57 | 110.29 | 50.17 | 240.56 | 0.8330 | 340.0 | 288.1 | |
| 0.00 | 2.05 | 0.00 | 1.83 | -19.85 | 110.35 | 50.24 | 240.29 | 0.8346 | 452.0 | 339.1 | |
| 0.00 | 1.16 | 0.00 | 0.94 | -19.92 | 105.76 | 45.65 | 237.95 | 0.7953 | 676.0 | 524.8 | |
| 0.36 | 1.34 | 0.29 | 1.09 | -20.56 | 105.45 | 45.33 | 237.06 | 0.7956 | 621.5 | 548.9 | |
| 0.00 | 0.71 | 0.00 | 0.58 | -20.96 | 105.37 | 45.26 | 236.58 | 0.7969 | 392.0 | 333.4 | |
| 0.00 | 1.51 | 0.00 | 1.25 | -22.96 | 104.84 | 44.72 | 234.08 | 0.8023 | 550.0 | 529.0 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -18.78 | 103.17 | 43.05 | 237.83 | 0.7658 | -364.0 | -341.0 | |
| 0.00 | 0.45 | 0.00 | 0.33 | -17.00 | 102.50 | 42.39 | 239.55 | 0.7502 | -558.0 | -522.6 | |
| 0.00 | 1.96 | 0.00 | 1.49 | -18.75 | 102.85 | 42.74 | 237.68 | 0.7627 | -293.0 | -263.4 | |
| 0.00 | 0.71 | 0.00 | 0.54 | -18.94 | 102.78 | 42.67 | 237.42 | 0.7630 | -461.0 | -424.4 | |
| 0.00 | 0.80 | 0.00 | 0.61 | -18.93 | 102.30 | 42.19 | 237.15 | 0.7584 | -608.0 | -532.2 | |
| 0.00 | 0.98 | 0.00 | 0.74 | -19.09 | 102.18 | 42.06 | 236.89 | 0.7581 | -584.0 | -431.9 | |
| 0.00 | 0.62 | 0.00 | 0.47 | -19.21 | 102.09 | 41.97 | 236.69 | 0.7579 | -554.0 | -472.7 | |
| 0.00 | 1.34 | 0.00 | 1.00 | -18.86 | 101.89 | 41.78 | 236.99 | 0.7541 | -710.0 | -577.9 | |
| 0.00 | 0.62 | 0.00 | 0.48 | -26.41 | 98.40 | 38.29 | 226.33 | 0.7695 | -485.0 | -406.1 | |
| 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. | |