SDO HMI 2014-09-26 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.77 | 19.43 | 1.66 | 18.50 | -14.46 | 185.17 | -55.10 | 111.60 | 0.8560 | 49.7 | -43.8 | |
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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 | 1.59 | 0.00 | 1.45 | -14.36 | 186.73 | -53.54 | 112.04 | 0.8427 | 522.0 | 418.1 | |
| 0.00 | 0.53 | 0.00 | 0.48 | -13.50 | 187.02 | -53.25 | 111.17 | 0.8376 | 642.0 | 576.0 | |
| 0.44 | 1.59 | 0.40 | 1.45 | -14.18 | 186.64 | -53.63 | 111.80 | 0.8430 | 537.8 | 494.6 | |
| 0.00 | 0.88 | 0.00 | 0.80 | -13.42 | 186.84 | -53.43 | 111.02 | 0.8390 | 469.0 | 377.4 | |
| 0.00 | 0.79 | 0.00 | 0.73 | -13.98 | 186.39 | -53.88 | 111.49 | 0.8445 | 287.0 | 346.4 | |
| 0.00 | 1.50 | 0.00 | 1.38 | -13.21 | 186.12 | -54.15 | 110.53 | 0.8447 | 446.0 | 379.5 | |
| 0.71 | 2.56 | 0.65 | 2.37 | -13.11 | 185.89 | -54.38 | 110.33 | 0.8464 | 406.5 | 356.4 | |
| 0.62 | 2.21 | 0.61 | 2.18 | -15.70 | 184.20 | -56.07 | 112.65 | 0.8675 | -584.3 | -481.3 | |
| 0.00 | 1.24 | 0.00 | 1.18 | -14.04 | 184.86 | -55.41 | 111.03 | 0.8577 | -556.0 | -434.7 | |
| 0.00 | 2.30 | 0.00 | 2.28 | -15.57 | 183.98 | -56.29 | 112.43 | 0.8689 | -456.0 | -314.8 | |
| 0.00 | 2.56 | 0.00 | 2.53 | -15.24 | 184.06 | -56.21 | 112.09 | 0.8674 | -551.0 | -497.2 | |
| 0.00 | 0.97 | 0.00 | 0.97 | -14.79 | 183.73 | -56.54 | 111.49 | 0.8689 | -420.0 | -307.6 | |
| 0.00 | 0.71 | 0.00 | 0.70 | -14.58 | 183.59 | -56.68 | 111.21 | 0.8695 | -414.0 | -406.9 | |
| 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. | |