SDO HMI 2014-12-03 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.46 | 60.01 | 34.65 | 75.96 | -15.91 | 127.10 | 65.76 | 252.34 | 0.9203 | 167.6 | 33.8 | |
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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 |
| 7.17 | 12.89 | 11.12 | 20.02 | -15.13 | 131.86 | 70.52 | 253.82 | 0.9490 | 337.4 | 129.8 | |
| 11.10 | 27.91 | 13.87 | 35.00 | -15.14 | 126.96 | 65.63 | 253.23 | 0.9200 | 357.1 | 62.4 | |
| 4.27 | -2.00 | 5.41 | -2.00 | -15.60 | 127.25 | 65.91 | 252.77 | 0.9223 | -316.0 | 999999 | |
| 0.00 | 1.88 | 0.00 | 2.27 | -15.25 | 126.07 | 64.73 | 252.99 | 0.9142 | 496.0 | 408.4 | |
| 0.43 | 1.54 | 0.50 | 1.80 | -17.09 | 124.90 | 63.56 | 250.81 | 0.9080 | 392.8 | 239.7 | |
| 0.00 | 1.28 | 0.00 | 1.50 | -17.28 | 124.80 | 63.46 | 250.59 | 0.9076 | 514.0 | 420.3 | |
| 0.00 | 1.54 | 0.00 | 1.67 | -16.39 | 122.80 | 61.46 | 251.23 | 0.8921 | -467.0 | -372.9 | |
| 0.51 | 1.71 | 0.58 | 1.93 | -19.80 | 123.36 | 62.02 | 247.58 | 0.9007 | 336.8 | 246.1 | |
| 2.13 | 8.11 | 2.27 | 8.59 | -17.71 | 121.86 | 60.53 | 249.58 | 0.8868 | -446.1 | -474.3 | |
| 0.85 | -9.00 | 0.90 | -9.00 | -17.46 | 121.66 | 60.32 | 249.82 | 0.8849 | -611.2 | 999999 | |
| 0.00 | 1.02 | 0.00 | 1.08 | -19.30 | 121.28 | 59.94 | 247.70 | 0.8848 | 341.0 | 320.6 | |
| 0.00 | 1.02 | 0.00 | 1.09 | -19.81 | 121.53 | 60.19 | 247.19 | 0.8875 | 491.0 | 398.8 | |
| 0.00 | 1.11 | 0.00 | 1.01 | -20.35 | 115.68 | 54.34 | 245.14 | 0.8417 | -611.0 | -525.2 | |
| 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. | |