SDO HMI 2014-12-11 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.05 | 292.05 | 33.03 | 175.19 | -3.94 | 1.10 | 34.20 | 263.58 | 0.5665 | 909.9 | 368.0 | |
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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 |
| 35.71 | 264.10 | 21.50 | 158.64 | -4.13 | 1.38 | 34.48 | 263.28 | 0.5708 | 1094.2 | 376.6 | |
| 0.68 | 3.49 | 0.41 | 2.10 | -1.38 | 1.29 | 34.40 | 268.12 | 0.5673 | -778.0 | -650.3 | |
| 1.87 | 11.68 | 1.12 | 6.96 | -2.92 | 0.83 | 33.93 | 265.35 | 0.5615 | 697.1 | 565.6 | |
| 13.72 | -1.00 | 8.20 | -1.00 | -3.87 | 0.80 | 33.90 | 263.66 | 0.5621 | 1243.9 | 999999 | |
| 0.26 | -1.00 | 0.15 | -1.00 | -4.22 | 0.78 | 33.88 | 263.02 | 0.5623 | 982.7 | 999999 | |
| 1.11 | -3.00 | 0.66 | -3.00 | -2.63 | 0.61 | 33.71 | 265.85 | 0.5580 | 607.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.81 | -1.83 | 0.27 | 33.37 | 267.26 | 0.5526 | -602.0 | -611.2 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -6.74 | 0.19 | 33.29 | 258.40 | 0.5586 | 645.0 | 479.6 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -2.84 | 359.73 | 32.83 | 265.38 | 0.5454 | 754.0 | 591.1 | |
| 0.00 | 1.87 | 0.00 | 1.10 | -2.75 | 359.13 | 32.23 | 265.47 | 0.5365 | 789.0 | 597.7 | |
| 0.00 | 3.24 | 0.00 | 1.89 | -1.98 | 358.87 | 31.97 | 266.88 | 0.5320 | 879.0 | 772.7 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -4.05 | 358.83 | 31.93 | 262.98 | 0.5336 | 732.0 | 562.2 | |
| 1.70 | 3.24 | 0.99 | 1.88 | -3.28 | 358.07 | 31.17 | 264.31 | 0.5214 | -812.1 | -682.4 | |
| 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. | |