SDO HMI 2014-10-05 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.18 | 0.00 | 13.64 | -17.76 | 101.83 | -21.34 | 139.96 | 0.5359 | 77.9 | -13.3 | |
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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 | 1.05 | 0.00 | 0.58 | -14.99 | 108.91 | -14.26 | 146.74 | 0.4356 | 716.0 | 606.6 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -16.97 | 108.60 | -14.57 | 148.63 | 0.4641 | 734.0 | 564.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -17.71 | 108.24 | -14.92 | 148.87 | 0.4765 | 730.0 | 595.0 | |
| 0.00 | 2.20 | 0.00 | 1.25 | -18.64 | 107.77 | -15.40 | 149.12 | 0.4923 | 545.0 | 541.3 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -17.41 | 106.11 | -17.06 | 145.05 | 0.4905 | 763.0 | 604.0 | |
| 0.00 | 2.81 | 0.00 | 1.59 | -17.12 | 106.07 | -17.09 | 144.63 | 0.4872 | 651.0 | 519.6 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -17.13 | 105.88 | -17.29 | 144.33 | 0.4891 | 816.0 | 716.2 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -16.71 | 105.72 | -17.45 | 143.55 | 0.4854 | 755.0 | 640.3 | |
| 0.00 | 3.07 | 0.00 | 1.83 | -17.59 | 99.27 | -23.90 | 135.92 | 0.5572 | -708.0 | -664.5 | |
| 0.00 | 1.76 | 0.00 | 1.07 | -19.19 | 98.30 | -24.87 | 136.83 | 0.5827 | -694.0 | -489.4 | |
| 0.00 | 1.93 | 0.00 | 1.16 | -17.34 | 98.41 | -24.76 | 134.59 | 0.5635 | -731.0 | -561.4 | |
| 0.00 | 0.53 | 0.00 | 0.37 | -30.63 | 95.29 | -27.88 | 145.81 | 0.7183 | -622.0 | -529.5 | |
| 0.00 | 1.49 | 0.00 | 0.91 | -18.31 | 97.42 | -25.74 | 134.75 | 0.5828 | -721.0 | -518.4 | |
| 0.00 | 1.23 | 0.00 | 0.79 | -20.20 | 93.11 | -30.06 | 132.78 | 0.6427 | -428.0 | -447.6 | |
| 0.00 | 1.76 | 0.00 | 1.06 | -13.24 | 94.24 | -28.93 | 124.52 | 0.5737 | -637.0 | -477.8 | |
| 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. | |