SDO HMI 2014-07-02 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.44 | 0.00 | 8.68 | -12.85 | 254.87 | -42.15 | 111.74 | 0.7056 | 325.3 | 277.4 | |
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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 | 1.54 | 0.00 | 1.01 | -12.07 | 258.66 | -38.37 | 112.33 | 0.6585 | 130.0 | 149.7 | |
| 0.00 | 1.63 | 0.00 | 1.09 | -12.57 | 257.60 | -39.42 | 112.54 | 0.6734 | 705.0 | 601.9 | |
| 0.00 | 0.82 | 0.00 | 0.55 | -12.96 | 257.37 | -39.66 | 112.97 | 0.6778 | 511.0 | 455.4 | |
| 0.00 | 0.91 | 0.00 | 0.62 | -12.67 | 255.86 | -41.17 | 111.87 | 0.6943 | 510.0 | 465.5 | |
| 0.00 | 1.54 | 0.00 | 1.07 | -13.15 | 255.55 | -41.48 | 112.40 | 0.6998 | 455.0 | 397.5 | |
| 0.00 | 0.91 | 0.00 | 0.63 | -12.51 | 255.01 | -42.02 | 111.29 | 0.7036 | 654.0 | 507.6 | |
| 0.00 | 1.54 | 0.00 | 1.08 | -13.03 | 254.52 | -42.51 | 111.79 | 0.7112 | 372.0 | 313.2 | |
| 0.00 | 0.91 | 0.00 | 0.63 | -11.73 | 254.74 | -42.28 | 110.12 | 0.7038 | 629.0 | 553.2 | |
| 0.00 | 0.91 | 0.00 | 0.66 | -11.54 | 252.15 | -44.88 | 108.89 | 0.7329 | 651.0 | 447.4 | |
| 0.00 | 1.00 | 0.00 | 0.78 | -14.85 | 249.37 | -47.65 | 112.11 | 0.7734 | -649.0 | -536.1 | |
| 0.00 | 0.73 | 0.00 | 0.56 | -14.43 | 249.45 | -47.58 | 111.62 | 0.7713 | -390.0 | -443.6 | |
| 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. | |