SDO HMI 2014-08-16 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.94 | 0.00 | 10.44 | -5.15 | 26.24 | -43.23 | 104.31 | 0.7051 | 294.5 | 201.5 | |
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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 | 1.35 | 0.00 | 0.89 | -4.52 | 29.69 | -39.78 | 104.72 | 0.6617 | 676.0 | 527.3 | |
| 0.00 | 1.17 | 0.00 | 0.78 | -4.87 | 29.50 | -39.96 | 105.16 | 0.6653 | 590.0 | 537.2 | |
| 0.00 | 1.26 | 0.00 | 0.83 | -4.68 | 29.51 | -39.95 | 104.89 | 0.6645 | 766.0 | 639.2 | |
| 0.00 | 1.35 | 0.00 | 0.90 | -4.89 | 29.22 | -40.24 | 105.07 | 0.6689 | 591.0 | 464.7 | |
| 0.00 | 1.35 | 0.00 | 0.90 | -3.04 | 28.45 | -41.01 | 102.10 | 0.6725 | 58.0 | 69.3 | |
| 0.00 | 1.17 | 0.00 | 0.79 | -5.03 | 28.24 | -41.22 | 104.88 | 0.6815 | 476.0 | 332.7 | |
| 0.00 | 1.26 | 0.00 | 0.85 | -4.09 | 27.98 | -41.48 | 103.45 | 0.6816 | 726.0 | 607.8 | |
| 0.00 | 0.99 | 0.00 | 0.72 | -6.13 | 24.23 | -45.24 | 104.89 | 0.7328 | -676.0 | -602.5 | |
| 0.00 | 2.16 | 0.00 | 1.60 | -6.71 | 23.24 | -46.23 | 105.30 | 0.7458 | -167.0 | -169.2 | |
| 0.00 | 1.71 | 0.00 | 1.27 | -4.79 | 22.51 | -46.95 | 102.56 | 0.7484 | -73.0 | -129.1 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -6.88 | 20.62 | -48.84 | 104.63 | 0.7748 | 273.0 | 322.8 | |
| 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. | |