SDO HMI 2014-01-09 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.12 | 0.00 | 7.91 | -21.74 | 107.69 | 29.03 | 232.70 | 0.5583 | -22.3 | 14.1 | |
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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 | 1.19 | 0.00 | 0.80 | -19.28 | 118.91 | 40.25 | 245.37 | 0.6733 | 572.0 | 443.8 | |
| 0.00 | 0.77 | 0.00 | 0.51 | -19.50 | 118.69 | 40.03 | 244.97 | 0.6716 | 561.0 | 521.3 | |
| 0.00 | 1.53 | 0.00 | 1.02 | -19.45 | 118.51 | 39.85 | 244.97 | 0.6693 | 446.0 | 475.7 | |
| 0.00 | 1.11 | 0.00 | 0.72 | -20.96 | 116.29 | 37.63 | 241.80 | 0.6494 | 590.0 | 485.3 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -21.68 | 115.31 | 36.65 | 240.25 | 0.6413 | 620.0 | 568.5 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -23.36 | 111.32 | 32.66 | 235.37 | 0.6044 | 593.0 | 514.7 | |
| 0.00 | 1.28 | 0.00 | 0.70 | -19.63 | 99.44 | 20.78 | 230.61 | 0.4343 | -624.0 | -506.8 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -19.48 | 99.42 | 20.76 | 230.88 | 0.4326 | -667.0 | -424.8 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -24.94 | 95.49 | 16.83 | 216.05 | 0.4481 | -807.0 | -638.4 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -24.98 | 95.33 | 16.67 | 215.74 | 0.4470 | -828.0 | -700.2 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -25.64 | 95.39 | 16.73 | 214.89 | 0.4556 | -701.0 | -521.1 | |
| 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. | |