SDO HMI 2014-07-02 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.56 | 0.00 | 10.80 | -13.29 | 254.19 | -45.61 | 110.90 | 0.7455 | 318.3 | 184.5 | |
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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 | 0.82 | 0.00 | 0.57 | -12.68 | 257.78 | -42.02 | 111.50 | 0.7042 | 679.0 | 605.9 | |
| 0.00 | 2.45 | 0.00 | 1.72 | -12.88 | 257.49 | -42.31 | 111.65 | 0.7083 | 644.0 | 371.7 | |
| 0.00 | 0.73 | 0.00 | 0.51 | -12.59 | 257.46 | -42.34 | 111.25 | 0.7076 | 677.0 | 556.5 | |
| 0.00 | 0.73 | 0.00 | 0.51 | -12.71 | 256.71 | -43.09 | 111.11 | 0.7166 | 541.0 | 430.0 | |
| 0.00 | 0.82 | 0.00 | 0.58 | -12.43 | 256.68 | -43.12 | 110.72 | 0.7159 | 387.0 | 351.6 | |
| 0.00 | 0.82 | 0.00 | 0.60 | -12.50 | 254.93 | -44.87 | 110.13 | 0.7359 | 689.0 | 554.2 | |
| 0.00 | 0.91 | 0.00 | 0.66 | -12.66 | 254.85 | -44.95 | 110.31 | 0.7373 | 392.0 | 437.4 | |
| 0.00 | 0.73 | 0.00 | 0.53 | -12.79 | 254.77 | -45.03 | 110.45 | 0.7386 | 543.0 | 545.1 | |
| 0.00 | 1.27 | 0.00 | 0.93 | -11.68 | 254.75 | -45.05 | 109.00 | 0.7353 | 674.0 | 574.6 | |
| 0.00 | 0.27 | 0.00 | 0.20 | -12.80 | 254.41 | -45.39 | 110.33 | 0.7426 | 438.0 | 407.3 | |
| 0.00 | 0.91 | 0.00 | 0.67 | -12.68 | 254.26 | -45.54 | 110.12 | 0.7438 | 426.0 | 340.1 | |
| 0.00 | 1.73 | 0.00 | 1.38 | -15.32 | 250.89 | -48.91 | 112.24 | 0.7875 | -482.0 | -363.3 | |
| 0.00 | 1.73 | 0.00 | 1.42 | -14.68 | 249.33 | -50.47 | 110.94 | 0.8011 | -517.0 | -470.6 | |
| 0.00 | 0.64 | 0.00 | 0.52 | -14.33 | 249.44 | -50.36 | 110.55 | 0.7990 | -635.0 | -534.6 | |
| 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. | |