SDO HMI 2014-08-19 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.48 | 109.89 | 26.86 | 120.95 | -9.51 | 331.22 | -61.34 | 104.28 | 0.8947 | 500.0 | 196.7 | |
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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 | 0.63 | 0.00 | 0.59 | -10.66 | 336.95 | -55.61 | 107.11 | 0.8506 | 207.0 | 261.9 | |
| 0.00 | 1.26 | 0.00 | 1.17 | -9.34 | 336.97 | -55.59 | 105.60 | 0.8473 | 522.0 | 478.1 | |
| 19.17 | 95.22 | 20.86 | 104.34 | -9.52 | 331.55 | -61.01 | 104.37 | 0.8924 | 758.2 | 219.9 | |
| 0.00 | 1.44 | 0.00 | 1.66 | -11.23 | 330.23 | -62.33 | 105.91 | 0.9050 | 406.0 | 311.9 | |
| 0.00 | 1.89 | 0.00 | 2.13 | -9.75 | 330.56 | -62.00 | 104.38 | 0.9001 | -286.0 | -248.8 | |
| 4.95 | -3.00 | 5.56 | -3.00 | -9.40 | 330.61 | -61.95 | 104.01 | 0.8992 | 404.6 | 999999 | |
| 0.00 | 0.90 | 0.00 | 1.02 | -9.28 | 330.25 | -62.31 | 103.80 | 0.9016 | 226.0 | 217.5 | |
| 0.00 | 1.89 | 0.00 | 2.16 | -9.49 | 330.05 | -62.51 | 103.98 | 0.9034 | 140.0 | 92.2 | |
| 0.00 | 0.63 | 0.00 | 0.76 | -11.06 | 328.92 | -63.63 | 105.40 | 0.9138 | -159.0 | -148.4 | |
| 0.00 | 1.44 | 0.00 | 1.67 | -8.76 | 329.53 | -63.03 | 103.07 | 0.9060 | 128.0 | 181.2 | |
| 0.36 | 1.35 | 0.44 | 1.65 | -10.79 | 328.46 | -64.09 | 105.01 | 0.9165 | -397.8 | -363.2 | |
| 0.00 | 1.71 | 0.00 | 1.97 | -7.49 | 329.49 | -63.07 | 101.68 | 0.9044 | 53.0 | 117.2 | |
| 0.00 | 1.53 | 0.00 | 1.83 | -9.34 | 328.86 | -63.70 | 103.54 | 0.9116 | 201.0 | 152.2 | |
| 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. | |