SDO HMI 2014-07-02 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.90 | 0.00 | 9.22 | -12.65 | 255.53 | -43.72 | 110.78 | 0.7231 | 459.1 | 405.5 | |
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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 | 0.64 | 0.00 | 0.44 | -12.89 | 257.44 | -41.80 | 111.88 | 0.7025 | 570.0 | 502.4 | |
| 0.00 | 0.91 | 0.00 | 0.63 | -12.57 | 257.47 | -41.78 | 111.46 | 0.7010 | 755.0 | 666.3 | |
| 0.00 | 1.54 | 0.00 | 1.07 | -12.39 | 257.25 | -42.00 | 111.12 | 0.7028 | 664.0 | 521.0 | |
| 0.00 | 1.00 | 0.00 | 0.69 | -11.60 | 257.24 | -42.01 | 110.04 | 0.7001 | 461.0 | 392.4 | |
| 0.00 | 0.91 | 0.00 | 0.64 | -12.63 | 256.69 | -42.55 | 111.22 | 0.7102 | 423.0 | 349.6 | |
| 0.00 | 0.45 | 0.00 | 0.32 | -13.17 | 256.58 | -42.67 | 111.90 | 0.7135 | 481.0 | 423.8 | |
| 0.00 | 1.27 | 0.00 | 0.90 | -12.72 | 255.86 | -43.39 | 111.00 | 0.7200 | 461.0 | 474.6 | |
| 0.00 | 0.54 | 0.00 | 0.39 | -12.80 | 255.36 | -43.88 | 110.91 | 0.7259 | 549.0 | 478.2 | |
| 0.00 | 2.09 | 0.00 | 1.51 | -12.73 | 254.86 | -44.39 | 110.62 | 0.7313 | 498.0 | 426.5 | |
| 0.00 | 1.09 | 0.00 | 0.78 | -11.69 | 254.91 | -44.34 | 109.26 | 0.7273 | 655.0 | 510.9 | |
| 0.00 | 1.00 | 0.00 | 0.73 | -12.61 | 254.66 | -44.58 | 110.39 | 0.7331 | 535.0 | 448.8 | |
| 0.00 | 0.73 | 0.00 | 0.53 | -12.81 | 254.40 | -44.85 | 110.55 | 0.7367 | 449.0 | 379.4 | |
| 0.00 | 0.73 | 0.00 | 0.59 | -14.69 | 249.28 | -49.97 | 111.11 | 0.7962 | -533.0 | -463.4 | |
| 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. | |