SDO HMI 2014-11-08 20:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.36 | 25.51 | 1.78 | 13.72 | -14.70 | 19.70 | -12.83 | 146.73 | 0.3822 | 89.3 | 106.6 | |
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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 | 1.81 | 0.00 | 0.93 | -11.77 | 28.23 | -4.31 | 164.48 | 0.2760 | 881.0 | 645.9 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -13.66 | 23.92 | -8.62 | 153.79 | 0.3311 | 900.0 | 651.1 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -14.50 | 23.23 | -9.30 | 153.20 | 0.3486 | 642.0 | 554.9 | |
| 2.07 | 3.79 | 1.09 | 1.99 | -12.95 | 22.58 | -9.95 | 149.32 | 0.3315 | 1180.6 | 906.5 | |
| 0.00 | 3.45 | 0.00 | 1.81 | -13.21 | 22.33 | -10.21 | 149.08 | 0.3372 | 727.0 | 758.4 | |
| 0.00 | 2.07 | 0.00 | 1.09 | -12.93 | 22.34 | -10.19 | 148.66 | 0.3332 | 733.0 | 681.2 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -14.21 | 21.31 | -11.22 | 148.23 | 0.3598 | 845.0 | 731.2 | |
| 1.29 | 2.93 | 0.69 | 1.57 | -14.39 | 19.83 | -12.70 | 145.26 | 0.3753 | -1044.9 | -795.9 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -16.30 | 15.84 | -16.69 | 140.76 | 0.4378 | -791.0 | -687.4 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -18.71 | 14.42 | -18.11 | 141.97 | 0.4800 | -741.0 | -682.9 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -18.94 | 14.23 | -18.30 | 141.99 | 0.4844 | -438.0 | -490.4 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -17.69 | 14.17 | -18.36 | 140.18 | 0.4706 | -684.0 | -570.5 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -18.59 | 14.00 | -18.53 | 141.19 | 0.4825 | -606.0 | -574.3 | |
| 0.00 | 2.50 | 0.00 | 1.41 | -16.34 | 11.94 | -20.59 | 134.97 | 0.4789 | -803.0 | -539.2 | |
| 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. | |