SDO HMI 2014-11-12 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.73 | 67.97 | 11.09 | 38.30 | -8.84 | 323.23 | -25.89 | 115.22 | 0.4789 | 877.5 | 528.6 | |
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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 |
| 0.00 | 0.69 | 0.00 | 0.39 | -12.61 | 323.35 | -25.77 | 122.19 | 0.5033 | 560.0 | 383.4 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -11.16 | 323.47 | -25.65 | 119.75 | 0.4912 | 742.0 | 574.7 | |
| 8.27 | 54.26 | 4.64 | 30.52 | -8.75 | 323.58 | -25.54 | 115.33 | 0.4735 | 1192.5 | 518.7 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -11.47 | 323.24 | -25.88 | 120.09 | 0.4965 | 617.0 | 506.4 | |
| 7.41 | -3.00 | 4.17 | -3.00 | -8.66 | 323.35 | -25.77 | 114.98 | 0.4761 | 1080.2 | 999999 | |
| 4.05 | -3.00 | 2.28 | -3.00 | -8.67 | 323.11 | -26.01 | 114.79 | 0.4794 | 843.2 | 999999 | |
| 0.00 | 3.79 | 0.00 | 2.14 | -8.49 | 322.86 | -26.26 | 114.25 | 0.4819 | 620.0 | 553.4 | |
| 0.00 | 2.50 | 0.00 | 1.42 | -9.65 | 322.70 | -26.42 | 116.30 | 0.4913 | 764.0 | 677.5 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -9.51 | 322.27 | -26.85 | 115.68 | 0.4962 | 612.0 | 481.8 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -9.36 | 322.05 | -27.07 | 115.23 | 0.4984 | 665.0 | 515.3 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -9.61 | 321.86 | -27.26 | 115.53 | 0.5025 | 516.0 | 423.2 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -7.83 | 321.73 | -27.39 | 112.11 | 0.4939 | 808.0 | 681.0 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -7.68 | 321.51 | -27.61 | 111.68 | 0.4963 | 642.0 | 458.5 | |
| 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. | |