SDO HMI 2014-12-07 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.11 | 0.00 | 9.86 | 14.48 | 16.17 | -1.26 | 1.24 | 0.2612 | -638.4 | -527.9 | |
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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 | 3.07 | 0.00 | 1.56 | 12.57 | 21.31 | 3.88 | 342.99 | 0.2269 | -649.0 | -659.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.30 | 20.59 | 3.16 | 346.76 | 0.2357 | -765.0 | -621.2 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 18.58 | 19.68 | 2.26 | 353.28 | 0.3207 | -816.0 | -664.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 13.18 | 18.92 | 1.49 | 353.60 | 0.2288 | -758.0 | -622.3 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 10.44 | 18.30 | 0.87 | 355.22 | 0.1809 | -979.0 | -689.9 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 22.11 | 18.05 | 0.62 | 358.46 | 0.3767 | -755.0 | -577.2 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 12.61 | 17.40 | -0.02 | 0.11 | 0.2176 | -863.0 | -701.9 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 12.18 | 17.25 | -0.18 | 0.82 | 0.2104 | -1051.0 | -913.4 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 8.13 | 17.16 | -0.27 | 1.89 | 0.1405 | -786.0 | -607.5 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 12.39 | 17.16 | -0.27 | 1.22 | 0.2140 | -1023.0 | -696.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 13.15 | 17.01 | -0.42 | 1.80 | 0.2270 | -783.0 | -648.4 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 15.59 | 13.20 | -4.22 | 14.87 | 0.2777 | -840.0 | -664.8 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 20.14 | 4.30 | -13.12 | 31.88 | 0.4053 | 599.0 | 420.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 24.55 | 358.97 | -18.45 | 34.81 | 0.5063 | 532.0 | 476.2 | |
| 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. | |