SDO HMI 2014-11-16 18:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.65 | 27.06 | 9.55 | 31.38 | -12.35 | 224.82 | -63.35 | 105.03 | 0.9048 | -83.7 | 95.9 | |
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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 |
| 0.00 | 0.69 | 0.00 | 0.63 | -9.90 | 231.88 | -56.29 | 103.54 | 0.8450 | -314.0 | -221.6 | |
| 0.00 | 1.29 | 0.00 | 1.33 | -13.51 | 228.60 | -59.57 | 107.01 | 0.8787 | 371.0 | 268.0 | |
| 0.52 | 1.63 | 0.53 | 1.68 | -12.84 | 228.44 | -59.72 | 106.22 | 0.8789 | 448.5 | 456.9 | |
| 0.00 | 1.29 | 0.00 | 1.38 | -13.78 | 227.37 | -60.80 | 107.05 | 0.8887 | 354.0 | 157.9 | |
| 0.00 | 1.12 | 0.00 | 1.15 | -11.41 | 228.25 | -59.92 | 104.58 | 0.8784 | 284.0 | 238.4 | |
| 0.00 | 0.43 | 0.00 | 0.45 | -11.10 | 227.62 | -60.54 | 104.12 | 0.8830 | 374.0 | 403.4 | |
| 0.00 | 1.03 | 0.00 | 1.11 | -11.93 | 226.81 | -61.36 | 104.90 | 0.8904 | 339.0 | 268.2 | |
| 0.00 | 1.03 | 0.00 | 1.15 | -13.27 | 226.18 | -61.99 | 106.27 | 0.8970 | -516.0 | -452.2 | |
| 0.00 | 0.86 | 0.00 | 0.97 | -13.78 | 225.88 | -62.29 | 106.77 | 0.8998 | -397.0 | -359.2 | |
| 0.00 | 4.64 | 0.00 | 4.99 | -11.35 | 226.78 | -61.39 | 104.25 | 0.8899 | 485.0 | 333.1 | |
| 0.77 | 2.06 | 0.97 | 2.58 | -12.16 | 222.75 | -65.42 | 104.47 | 0.9198 | -567.3 | -505.8 | |
| 6.36 | 8.93 | 8.05 | 11.31 | -12.54 | 222.49 | -65.68 | 104.84 | 0.9219 | -387.8 | -131.7 | |
| 0.00 | 1.12 | 0.00 | 1.43 | -12.28 | 222.17 | -66.00 | 104.51 | 0.9237 | 344.0 | 274.5 | |
| 0.00 | 0.94 | 0.00 | 1.22 | -12.50 | 222.06 | -66.11 | 104.73 | 0.9247 | 391.0 | 358.0 | |
| 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. | |