SDO HMI 2014-11-23 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.13 | 0.00 | 10.45 | -12.38 | 225.71 | 20.50 | 234.23 | 0.4222 | 49.9 | 59.2 | |
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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 | 0.34 | 0.00 | 0.19 | -13.53 | 229.03 | 23.82 | 236.13 | 0.4748 | 427.0 | 328.2 | |
| 0.00 | 1.89 | 0.00 | 1.05 | -13.10 | 228.49 | 23.27 | 236.34 | 0.4643 | 676.0 | 574.9 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -12.05 | 228.36 | 23.14 | 238.15 | 0.4544 | 714.0 | 590.2 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -13.62 | 228.41 | 23.19 | 235.29 | 0.4676 | 590.0 | 449.6 | |
| 0.00 | 2.23 | 0.00 | 1.24 | -12.85 | 228.23 | 23.02 | 236.52 | 0.4590 | 943.0 | 848.8 | |
| 0.00 | 2.06 | 0.00 | 1.15 | -13.55 | 228.07 | 22.86 | 235.04 | 0.4627 | 811.0 | 686.1 | |
| 0.00 | 1.37 | 0.00 | 0.76 | -13.45 | 227.27 | 22.05 | 234.29 | 0.4516 | 785.0 | 604.9 | |
| 0.00 | 1.80 | 0.00 | 0.97 | -12.94 | 223.72 | 18.51 | 230.54 | 0.4024 | -850.0 | -635.8 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -10.80 | 223.38 | 18.17 | 234.50 | 0.3779 | -852.0 | -700.8 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -11.44 | 223.39 | 18.18 | 233.13 | 0.3839 | -771.0 | -552.0 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -11.77 | 223.25 | 18.04 | 232.22 | 0.3853 | -852.0 | -730.7 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -11.44 | 223.20 | 17.99 | 232.85 | 0.3814 | -758.0 | -613.3 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -12.17 | 223.12 | 17.91 | 231.20 | 0.3874 | -799.0 | -698.1 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -8.62 | 219.70 | 14.49 | 233.71 | 0.3083 | 634.0 | 482.8 | |
| 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. | |