SDO HMI 2014-11-16 16:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.42 | 29.98 | 10.63 | 36.12 | -12.42 | 224.83 | -64.44 | 104.92 | 0.9127 | -87.9 | -37.3 | |
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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 | 1.12 | 0.00 | 1.19 | -13.59 | 228.67 | -60.61 | 106.88 | 0.8869 | 232.0 | 225.5 | |
| 0.00 | 0.77 | 0.00 | 0.82 | -13.01 | 228.60 | -60.67 | 106.22 | 0.8866 | 374.0 | 358.6 | |
| 1.20 | 2.06 | 1.28 | 2.20 | -12.83 | 228.42 | -60.85 | 105.99 | 0.8877 | 409.8 | 347.9 | |
| 0.52 | 1.98 | 0.57 | 2.19 | -13.76 | 227.37 | -61.90 | 106.82 | 0.8970 | 134.5 | 85.4 | |
| 0.34 | 1.55 | 0.37 | 1.65 | -11.40 | 228.17 | -61.11 | 104.36 | 0.8878 | 195.2 | 195.8 | |
| 0.00 | 1.03 | 0.00 | 1.12 | -11.09 | 227.71 | -61.56 | 103.93 | 0.8910 | 310.0 | 285.2 | |
| 0.00 | 0.43 | 0.00 | 0.49 | -13.25 | 226.48 | -62.79 | 106.09 | 0.9028 | -238.0 | -224.2 | |
| 0.00 | 0.60 | 0.00 | 0.70 | -13.76 | 226.04 | -63.24 | 106.57 | 0.9066 | -435.0 | -391.4 | |
| 0.00 | 0.60 | 0.00 | 0.69 | -13.23 | 226.29 | -62.98 | 106.04 | 0.9042 | -275.0 | -356.3 | |
| 0.00 | 4.30 | 0.00 | 4.80 | -11.31 | 226.78 | -62.49 | 104.01 | 0.8983 | 516.0 | 290.3 | |
| 0.00 | 0.94 | 0.00 | 1.06 | -11.53 | 226.69 | -62.58 | 104.24 | 0.8992 | 161.0 | 175.4 | |
| 0.00 | 0.60 | 0.00 | 0.75 | -12.31 | 223.98 | -65.29 | 104.66 | 0.9191 | -491.0 | -424.1 | |
| 6.36 | 13.40 | 8.41 | 17.65 | -12.53 | 222.51 | -66.76 | 104.67 | 0.9288 | -383.6 | -366.2 | |
| 0.00 | 0.60 | 0.00 | 0.81 | -12.21 | 222.13 | -67.14 | 104.27 | 0.9309 | 301.0 | 263.4 | |
| 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. | |