SDO HMI 2014-07-02 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.24 | 0.00 | 7.23 | -12.20 | 254.72 | -42.86 | 110.59 | 0.7121 | 422.1 | 375.4 | |
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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 | 0.54 | 0.00 | 0.37 | -12.94 | 257.56 | -40.03 | 112.77 | 0.6821 | 560.0 | 611.3 | |
| 0.00 | 1.36 | 0.00 | 0.92 | -12.56 | 257.55 | -40.03 | 112.24 | 0.6806 | 736.0 | 629.2 | |
| 0.00 | 0.91 | 0.00 | 0.62 | -12.95 | 257.35 | -40.23 | 112.68 | 0.6845 | 450.0 | 396.3 | |
| 0.00 | 1.18 | 0.00 | 0.81 | -12.82 | 256.59 | -40.99 | 112.15 | 0.6929 | 420.0 | 327.1 | |
| 0.00 | 0.82 | 0.00 | 0.57 | -12.53 | 255.01 | -42.57 | 111.08 | 0.7101 | 649.0 | 505.8 | |
| 0.00 | 0.73 | 0.00 | 0.52 | -13.21 | 254.52 | -43.06 | 111.79 | 0.7181 | 418.0 | 297.2 | |
| 0.00 | 1.54 | 0.00 | 1.09 | -13.02 | 254.52 | -43.06 | 111.54 | 0.7175 | 453.0 | 335.4 | |
| 0.00 | 0.54 | 0.00 | 0.38 | -11.81 | 254.73 | -42.85 | 110.00 | 0.7107 | 467.0 | 484.8 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -11.50 | 252.14 | -45.45 | 108.63 | 0.7392 | 524.0 | 490.7 | |
| 0.00 | 1.63 | 0.00 | 1.19 | -9.11 | 251.65 | -45.93 | 105.32 | 0.7378 | 466.0 | 314.3 | |
| 0.00 | 0.45 | 0.00 | 0.36 | -14.84 | 249.31 | -48.27 | 111.88 | 0.7796 | -500.0 | -461.0 | |
| 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. | |