SDO HMI 2014-12-11 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.38 | 268.61 | 29.85 | 169.12 | -3.99 | 1.09 | 38.01 | 264.10 | 0.6198 | 907.8 | 331.8 | |
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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 |
| 0.68 | 2.73 | 0.43 | 1.72 | -1.55 | 1.45 | 38.37 | 268.04 | 0.6232 | -779.4 | -610.8 | |
| 31.28 | 249.62 | 19.77 | 157.41 | -4.13 | 1.36 | 38.28 | 263.90 | 0.6237 | 1103.4 | 350.9 | |
| 12.53 | -2.00 | 7.86 | -2.00 | -3.92 | 0.78 | 37.70 | 264.16 | 0.6156 | 1284.4 | 999999 | |
| 1.70 | 3.66 | 1.06 | 2.29 | -2.80 | 0.51 | 37.43 | 265.96 | 0.6109 | 808.2 | 674.1 | |
| 0.00 | 1.36 | 0.00 | 0.85 | -5.97 | 0.39 | 37.31 | 260.77 | 0.6131 | 454.0 | 431.6 | |
| 0.00 | 1.19 | 0.00 | 0.73 | -2.80 | 359.29 | 36.21 | 265.85 | 0.5938 | 716.0 | 519.7 | |
| 0.00 | 1.28 | 0.00 | 0.78 | -3.33 | 359.20 | 36.12 | 264.94 | 0.5930 | 689.0 | 490.5 | |
| 0.00 | 1.53 | 0.00 | 0.94 | -3.57 | 359.14 | 36.05 | 264.53 | 0.5924 | 964.0 | 793.8 | |
| 1.19 | 2.39 | 0.73 | 1.45 | -2.01 | 358.72 | 35.64 | 267.16 | 0.5852 | 778.1 | 605.8 | |
| 0.00 | 3.15 | 0.00 | 1.92 | -2.60 | 358.55 | 35.47 | 266.13 | 0.5833 | -764.0 | -503.7 | |
| 0.00 | 1.70 | 0.00 | 1.03 | -3.37 | 358.07 | 34.99 | 264.75 | 0.5771 | -824.0 | -688.0 | |
| 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. | |