SDO HMI 2014-12-09 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.55 | 0.00 | 10.16 | 14.23 | 17.83 | 33.35 | 295.44 | 0.5925 | -527.0 | -432.9 | |
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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 | 2.56 | 0.00 | 1.67 | 13.44 | 23.31 | 38.83 | 291.07 | 0.6559 | -502.0 | -411.2 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 10.20 | 20.98 | 36.50 | 287.07 | 0.6147 | -427.0 | -379.5 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 12.64 | 20.68 | 36.20 | 291.03 | 0.6197 | -732.0 | -637.6 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 12.76 | 20.66 | 36.18 | 291.23 | 0.6199 | -741.0 | -582.8 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 13.49 | 19.40 | 34.92 | 292.98 | 0.6069 | -597.0 | -472.2 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 11.55 | 17.90 | 33.41 | 290.62 | 0.5787 | -630.0 | -526.3 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 11.52 | 17.71 | 33.23 | 290.67 | 0.5761 | -770.0 | -647.2 | |
| 0.00 | 2.98 | 0.00 | 1.83 | 15.10 | 17.69 | 33.21 | 296.48 | 0.5930 | -628.0 | -572.9 | |
| 0.00 | 1.28 | 0.00 | 0.78 | 16.45 | 16.30 | 31.82 | 299.50 | 0.5832 | -590.0 | -393.7 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 17.04 | 15.29 | 30.81 | 301.14 | 0.5743 | -666.0 | -533.5 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 14.03 | 13.07 | 28.59 | 297.86 | 0.5272 | -627.0 | -463.2 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 15.47 | 12.97 | 28.49 | 300.39 | 0.5350 | -658.0 | -526.7 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 20.31 | 6.77 | 22.29 | 314.55 | 0.5011 | 717.0 | 480.9 | |
| 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. | |