SDO HMI 2014-10-14 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.78 | 359.54 | 54.34 | 295.27 | -8.96 | 319.55 | -50.91 | 106.03 | 0.7983 | 612.8 | 261.9 | |
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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 |
| 22.48 | 321.76 | 17.94 | 256.18 | -9.18 | 320.94 | -49.52 | 106.69 | 0.7861 | 956.8 | 320.4 | |
| 23.71 | -1.00 | 18.82 | -1.00 | -8.59 | 321.01 | -49.45 | 105.98 | 0.7838 | 1068.4 | 999999 | |
| 4.20 | -1.00 | 3.35 | -1.00 | -8.88 | 320.81 | -49.65 | 106.28 | 0.7867 | 1003.4 | 999999 | |
| 5.42 | -1.00 | 4.36 | -1.00 | -8.97 | 320.51 | -49.95 | 106.29 | 0.7900 | 552.5 | 999999 | |
| 2.45 | -1.00 | 1.99 | -1.00 | -9.22 | 320.13 | -50.33 | 106.47 | 0.7945 | 221.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.77 | -8.25 | 316.56 | -53.90 | 104.25 | 0.8272 | 444.0 | 381.4 | |
| 0.00 | 0.79 | 0.00 | 0.73 | -10.17 | 314.68 | -55.78 | 105.97 | 0.8487 | -544.0 | -389.3 | |
| 0.00 | 0.96 | 0.00 | 0.93 | -9.75 | 313.12 | -57.34 | 105.08 | 0.8613 | -602.0 | -491.6 | |
| 0.00 | 3.94 | 0.00 | 3.86 | -9.97 | 312.78 | -57.68 | 105.23 | 0.8647 | -634.0 | -488.5 | |
| 0.00 | 1.14 | 0.00 | 1.12 | -10.08 | 312.52 | -57.94 | 105.30 | 0.8671 | -511.0 | -426.8 | |
| 5.86 | 19.95 | 6.11 | 20.81 | -8.94 | 310.47 | -59.99 | 103.52 | 0.8818 | -592.2 | -163.8 | |
| 1.66 | 4.02 | 1.77 | 4.29 | -9.85 | 309.95 | -60.51 | 104.41 | 0.8874 | -371.6 | -213.5 | |
| 0.00 | 3.32 | 0.00 | 3.58 | -10.06 | 309.70 | -60.76 | 104.58 | 0.8897 | 362.0 | 269.4 | |
| 0.00 | 1.57 | 0.00 | 1.69 | -9.70 | 309.62 | -60.84 | 104.17 | 0.8897 | 357.0 | 294.8 | |
| 0.00 | 1.22 | 0.00 | 1.31 | -9.29 | 309.69 | -60.77 | 103.73 | 0.8885 | 124.0 | 161.7 | |
| 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. | |