SDO HMI 2014-08-11 18:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.63 | 59.14 | 8.29 | 38.88 | -17.97 | 161.84 | 33.43 | 232.92 | 0.6595 | 634.0 | 463.6 | |
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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 | 0.99 | 0.00 | 0.69 | -17.16 | 166.49 | 38.08 | 237.35 | 0.7023 | 532.0 | 392.6 | |
| 0.00 | 1.08 | 0.00 | 0.75 | -18.97 | 164.96 | 36.56 | 234.06 | 0.6980 | 493.0 | 290.8 | |
| 0.00 | 1.44 | 0.00 | 0.99 | -19.20 | 164.38 | 35.98 | 233.36 | 0.6937 | 394.0 | 352.6 | |
| 12.63 | 35.36 | 8.29 | 23.19 | -16.97 | 162.46 | 34.06 | 234.71 | 0.6585 | 952.0 | 516.6 | |
| 0.00 | 1.08 | 0.00 | 0.71 | -18.44 | 161.70 | 33.30 | 232.23 | 0.6611 | 547.0 | 482.0 | |
| 0.00 | 1.62 | 0.00 | 1.07 | -18.63 | 161.51 | 33.11 | 231.85 | 0.6605 | 717.0 | 646.4 | |
| 0.00 | 1.35 | 0.00 | 0.87 | -17.28 | 160.66 | 32.26 | 232.86 | 0.6415 | 754.0 | 516.7 | |
| 0.00 | 6.77 | 0.00 | 4.46 | -19.89 | 160.68 | 32.28 | 229.60 | 0.6617 | 566.0 | 559.1 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -19.87 | 160.41 | 32.01 | 229.40 | 0.6588 | 577.0 | 522.4 | |
| 0.00 | 1.80 | 0.00 | 1.18 | -19.48 | 160.17 | 31.77 | 229.66 | 0.6534 | 759.0 | 664.5 | |
| 0.00 | 1.08 | 0.00 | 0.71 | -19.47 | 159.98 | 31.58 | 229.51 | 0.6514 | 800.0 | 666.3 | |
| 0.00 | 1.89 | 0.00 | 1.24 | -20.53 | 159.68 | 31.28 | 227.96 | 0.6570 | 623.0 | 514.5 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -20.32 | 159.60 | 31.20 | 228.14 | 0.6545 | 691.0 | 660.5 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -19.69 | 158.11 | 29.71 | 227.56 | 0.6345 | -365.0 | -337.1 | |
| 0.00 | 1.80 | 0.00 | 1.15 | -20.58 | 157.18 | 28.78 | 225.59 | 0.6332 | -848.0 | -646.9 | |
| 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. | |