SDO HMI 2014-11-16 19:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.82 | 28.70 | 9.47 | 32.49 | -12.29 | 224.95 | -62.66 | 105.08 | 0.8999 | -35.7 | 111.7 | |
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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 | 1.55 | 0.00 | 1.57 | -13.43 | 228.55 | -59.06 | 107.02 | 0.8745 | 396.0 | 272.0 | |
| 0.86 | 2.15 | 0.87 | 2.17 | -12.82 | 228.49 | -59.12 | 106.32 | 0.8740 | 448.5 | 420.3 | |
| 0.00 | 1.03 | 0.00 | 1.09 | -13.76 | 227.38 | -60.24 | 107.14 | 0.8843 | 362.0 | 253.2 | |
| 0.00 | 0.60 | 0.00 | 0.61 | -11.43 | 228.23 | -59.39 | 104.69 | 0.8741 | 363.0 | 341.1 | |
| 0.00 | 1.03 | 0.00 | 1.04 | -10.97 | 228.08 | -59.53 | 104.15 | 0.8746 | 518.0 | 408.1 | |
| 0.00 | 0.94 | 0.00 | 0.97 | -11.08 | 227.68 | -59.93 | 104.20 | 0.8780 | 493.0 | 422.5 | |
| 0.00 | 1.37 | 0.00 | 1.50 | -13.32 | 226.19 | -61.43 | 106.42 | 0.8928 | -336.0 | -441.6 | |
| 0.00 | 1.55 | 0.00 | 1.64 | -11.88 | 226.78 | -60.84 | 104.93 | 0.8864 | 480.0 | 326.4 | |
| 0.00 | 0.52 | 0.00 | 0.57 | -13.54 | 226.02 | -61.59 | 106.63 | 0.8944 | -471.0 | -454.0 | |
| 0.00 | 4.98 | 0.00 | 5.27 | -11.36 | 226.78 | -60.83 | 104.36 | 0.8856 | 449.0 | 289.3 | |
| 0.86 | 2.41 | 1.05 | 2.95 | -12.17 | 222.76 | -64.85 | 104.57 | 0.9160 | -484.1 | -349.1 | |
| 6.10 | 8.59 | 7.55 | 10.64 | -12.52 | 222.52 | -65.09 | 104.91 | 0.9180 | -435.5 | -220.6 | |
| 0.00 | 0.86 | 0.00 | 1.07 | -11.98 | 222.34 | -65.27 | 104.30 | 0.9186 | 135.0 | 108.7 | |
| 0.00 | 1.12 | 0.00 | 1.40 | -12.26 | 222.14 | -65.48 | 104.57 | 0.9203 | 286.0 | 259.1 | |
| 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. | |