SDO HMI 2014-07-06 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.27 | 57.25 | 16.01 | 44.78 | -12.65 | 298.01 | 48.40 | 250.57 | 0.7758 | 85.7 | -49.6 | |
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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 |
| 5.00 | 22.90 | 4.02 | 18.43 | -12.87 | 299.31 | 49.70 | 250.71 | 0.7899 | 785.3 | 565.9 | |
| 7.63 | -1.00 | 6.15 | -1.00 | -13.28 | 299.27 | 49.66 | 250.20 | 0.7907 | 704.9 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.94 | -12.98 | 298.95 | 49.34 | 250.46 | 0.7866 | 535.0 | 568.1 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -13.09 | 298.54 | 48.93 | 250.20 | 0.7828 | 224.0 | 196.3 | |
| 0.00 | 0.73 | 0.00 | 0.57 | -12.99 | 297.85 | 48.24 | 250.08 | 0.7754 | -396.0 | -268.8 | |
| 2.27 | 8.00 | 1.75 | 6.15 | -11.84 | 297.38 | 47.77 | 251.38 | 0.7670 | -608.0 | -519.3 | |
| 0.64 | 5.27 | 0.49 | 4.08 | -12.86 | 297.58 | 47.97 | 250.17 | 0.7721 | -540.0 | -343.3 | |
| 0.00 | 1.09 | 0.00 | 0.83 | -11.64 | 297.15 | 47.54 | 251.56 | 0.7640 | -546.0 | -420.0 | |
| 1.91 | -7.00 | 1.47 | -7.00 | -12.91 | 297.31 | 47.70 | 250.01 | 0.7695 | -492.5 | 999999 | |
| 0.00 | 3.63 | 0.00 | 2.78 | -11.94 | 296.99 | 47.38 | 251.11 | 0.7632 | -529.0 | -402.3 | |
| 0.00 | 1.09 | 0.00 | 0.84 | -13.56 | 297.11 | 47.50 | 249.12 | 0.7694 | -472.0 | -411.5 | |
| 0.00 | 1.73 | 0.00 | 1.33 | -13.33 | 296.91 | 47.30 | 249.34 | 0.7666 | 337.0 | 375.1 | |
| 2.00 | 8.72 | 1.51 | 6.58 | -11.92 | 296.43 | 46.82 | 250.96 | 0.7571 | -675.0 | -516.8 | |
| 0.00 | 1.00 | 0.00 | 0.76 | -12.90 | 296.53 | 46.92 | 249.74 | 0.7611 | 225.0 | 153.1 | |
| 0.00 | 0.55 | 0.00 | 0.41 | -11.72 | 296.16 | 46.55 | 251.12 | 0.7535 | -610.0 | -445.2 | |
| 0.82 | -13.00 | 0.62 | -13.00 | -12.13 | 296.21 | 46.60 | 250.61 | 0.7553 | -677.8 | 999999 | |
| 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. | |