SDO HMI 2014-01-16 07:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.97 | 364.74 | 35.37 | 201.63 | -16.24 | 12.22 | 24.11 | 242.11 | 0.4454 | 985.3 | 423.6 | |
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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 |
| 31.22 | 211.20 | 17.38 | 117.65 | -16.56 | 13.07 | 24.96 | 242.19 | 0.4592 | 1186.5 | 386.5 | |
| 3.49 | -1.00 | 1.94 | -1.00 | -16.55 | 12.70 | 24.58 | 241.92 | 0.4539 | 1371.4 | 999999 | |
| 1.62 | -1.00 | 0.90 | -1.00 | -16.64 | 12.51 | 24.39 | 241.56 | 0.4519 | 1214.3 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.47 | -16.64 | 11.63 | 23.52 | 240.79 | 0.4399 | 543.0 | 377.9 | |
| 27.64 | 145.11 | 15.15 | 79.47 | -15.74 | 11.35 | 23.24 | 242.42 | 0.4303 | 1348.3 | 534.5 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -19.50 | 10.47 | 22.36 | 233.89 | 0.4458 | 592.0 | 514.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -15.20 | 7.19 | 19.08 | 239.35 | 0.3682 | -835.0 | -697.9 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -16.90 | 6.67 | 18.56 | 234.69 | 0.3749 | -707.0 | -537.6 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -16.17 | 5.22 | 17.10 | 234.32 | 0.3493 | -907.0 | -769.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -19.19 | 4.31 | 16.19 | 226.06 | 0.3673 | -881.0 | -674.9 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -12.32 | 3.41 | 15.30 | 242.21 | 0.2927 | -857.0 | -751.6 | |
| 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. | |