SDO HMI 2014-10-08 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.72 | 0.00 | 14.26 | -16.81 | 106.61 | 24.68 | 225.55 | 0.5632 | 147.9 | 306.4 | |
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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 | 2.98 | 0.00 | 1.79 | -13.40 | 110.39 | 28.46 | 235.02 | 0.5680 | 691.0 | 641.4 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -13.76 | 110.74 | 28.81 | 234.82 | 0.5749 | 614.0 | 533.0 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -13.34 | 109.95 | 28.02 | 234.68 | 0.5624 | 731.0 | 632.5 | |
| 0.00 | 6.22 | 0.00 | 3.73 | -13.53 | 110.14 | 28.21 | 234.59 | 0.5661 | 818.0 | 709.4 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -15.91 | 110.21 | 28.28 | 231.25 | 0.5864 | 660.0 | 539.0 | |
| 0.00 | 0.96 | 0.00 | 0.61 | -18.51 | 111.88 | 29.95 | 229.39 | 0.6258 | 664.0 | 568.2 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -18.68 | 107.56 | 25.63 | 224.82 | 0.5836 | 95.0 | 199.8 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -17.13 | 101.84 | 19.91 | 219.72 | 0.5112 | -622.0 | -566.6 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -16.45 | 100.68 | 18.75 | 218.95 | 0.4924 | -816.0 | -650.8 | |
| 0.00 | 1.31 | 0.00 | 0.84 | -22.35 | 108.85 | 26.92 | 221.78 | 0.6308 | 235.0 | 292.0 | |
| 0.00 | 1.23 | 0.00 | 0.78 | -22.58 | 108.32 | 26.39 | 220.98 | 0.6282 | 646.0 | 568.0 | |
| 0.00 | 1.40 | 0.00 | 0.89 | -23.46 | 107.14 | 25.21 | 218.74 | 0.6267 | 615.0 | 528.9 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -19.17 | 99.70 | 17.78 | 214.14 | 0.5159 | -664.0 | -535.9 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -18.26 | 89.36 | 7.43 | 196.48 | 0.4346 | -820.0 | -647.0 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -22.09 | 93.16 | 11.23 | 200.84 | 0.5090 | -628.0 | -523.1 | |
| 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. | |