SDO HMI 2014-10-06 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 19.05 | 0.37 | 13.99 | -17.74 | 77.39 | -41.36 | 121.39 | 0.7386 | 425.4 | 462.6 | |
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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 | 0.97 | 0.00 | 0.70 | -20.54 | 79.68 | -39.07 | 126.12 | 0.7330 | 451.0 | 414.3 | |
| 0.53 | 6.06 | 0.37 | 4.31 | -18.13 | 79.64 | -39.11 | 123.21 | 0.7189 | 895.7 | 674.5 | |
| 0.00 | 3.43 | 0.00 | 2.38 | -15.27 | 79.69 | -39.06 | 119.67 | 0.7019 | 733.0 | 611.8 | |
| 0.00 | 1.05 | 0.00 | 0.77 | -16.77 | 76.94 | -41.81 | 119.91 | 0.7388 | 734.0 | 628.8 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -19.54 | 75.80 | -42.95 | 122.58 | 0.7643 | 659.0 | 543.2 | |
| 0.00 | 2.72 | 0.00 | 2.02 | -16.83 | 76.20 | -42.55 | 119.57 | 0.7465 | 560.0 | 485.8 | |
| 0.00 | 0.70 | 0.00 | 0.54 | -19.39 | 75.19 | -43.56 | 122.06 | 0.7693 | 362.0 | 334.1 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -17.04 | 75.54 | -43.21 | 119.47 | 0.7542 | 502.0 | 414.1 | |
| 0.00 | 1.05 | 0.00 | 0.78 | -14.54 | 75.01 | -43.74 | 116.15 | 0.7478 | 529.0 | 366.1 | |
| 0.00 | 0.88 | 0.00 | 0.76 | -22.95 | 71.09 | -47.66 | 123.91 | 0.8223 | -451.0 | -359.5 | |
| 0.00 | 0.79 | 0.00 | 0.67 | -20.39 | 70.82 | -47.93 | 120.94 | 0.8135 | -469.0 | -411.9 | |
| 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. | |