SDO HMI 2014-07-03 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.43 | 37.49 | 12.61 | 30.00 | -16.02 | 233.05 | -48.52 | 113.37 | 0.7855 | -26.8 | 105.3 | |
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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 | 1.36 | 0.00 | 0.97 | -16.68 | 239.71 | -41.86 | 117.02 | 0.7199 | 555.0 | 488.9 | |
| 0.00 | 1.18 | 0.00 | 0.83 | -15.48 | 239.94 | -41.63 | 115.57 | 0.7120 | 637.0 | 512.8 | |
| 0.64 | 1.91 | 0.48 | 1.43 | -14.46 | 235.73 | -45.84 | 112.42 | 0.7537 | 627.6 | 580.7 | |
| 3.72 | 5.81 | 2.79 | 4.36 | -14.21 | 235.71 | -45.86 | 112.09 | 0.7531 | 828.0 | 606.1 | |
| 0.54 | 3.09 | 0.41 | 2.33 | -14.47 | 235.41 | -46.16 | 112.31 | 0.7572 | 674.2 | 492.7 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -14.76 | 235.33 | -46.24 | 112.65 | 0.7590 | -213.0 | -142.7 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -14.84 | 235.08 | -46.49 | 112.64 | 0.7619 | 415.0 | 342.3 | |
| 0.00 | 1.09 | 0.00 | 0.83 | -14.75 | 234.87 | -46.70 | 112.45 | 0.7638 | 406.0 | 306.9 | |
| 0.00 | 1.54 | 0.00 | 1.21 | -16.06 | 234.11 | -47.47 | 113.79 | 0.7761 | 563.0 | 460.1 | |
| 0.00 | 1.63 | 0.00 | 1.30 | -15.97 | 233.28 | -48.29 | 113.36 | 0.7841 | -608.0 | -500.6 | |
| 10.53 | 18.43 | 8.93 | 15.64 | -17.05 | 230.58 | -50.99 | 113.70 | 0.8135 | -730.6 | -242.1 | |
| 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. | |