SDO HMI 2014-12-05 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.46 | 0.00 | 9.63 | 14.00 | 17.32 | -29.19 | 63.47 | 0.5308 | -555.6 | -450.0 | |
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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 | 1.11 | 0.00 | 0.61 | 15.22 | 24.30 | -22.21 | 54.89 | 0.4477 | -800.0 | -630.8 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 16.35 | 20.11 | -26.40 | 57.14 | 0.5100 | -615.0 | -451.6 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 8.40 | 20.19 | -26.32 | 72.30 | 0.4623 | -530.0 | -477.5 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 15.39 | 19.08 | -27.43 | 59.69 | 0.5166 | -626.0 | -460.6 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 13.47 | 17.99 | -28.52 | 63.93 | 0.5190 | -720.0 | -529.1 | |
| 0.00 | 2.13 | 0.00 | 1.24 | 13.29 | 17.70 | -28.81 | 64.46 | 0.5219 | -734.0 | -635.0 | |
| 0.00 | 2.22 | 0.00 | 1.29 | 13.14 | 17.37 | -29.14 | 64.96 | 0.5254 | -432.0 | -407.6 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 13.65 | 17.20 | -29.31 | 64.17 | 0.5306 | -639.0 | -488.4 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 13.23 | 16.56 | -29.95 | 65.35 | 0.5369 | -653.0 | -454.6 | |
| 0.00 | 1.19 | 0.00 | 0.69 | 11.08 | 16.75 | -29.76 | 69.05 | 0.5237 | -783.0 | -662.8 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 13.71 | 15.96 | -30.55 | 64.90 | 0.5474 | -651.0 | -471.8 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 15.36 | 15.50 | -31.01 | 62.45 | 0.5626 | -660.0 | -521.8 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 20.72 | 8.67 | -37.84 | 58.72 | 0.6738 | 620.0 | 504.3 | |
| 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. | |