SDO HMI 2014-11-14 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.16 | 35.38 | 7.60 | 20.66 | 16.78 | 293.52 | -29.23 | 62.36 | 0.5297 | -308.8 | -193.8 | |
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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 |
| 10.15 | 22.98 | 5.85 | 13.24 | 16.43 | 294.64 | -28.11 | 62.19 | 0.5131 | -980.8 | -596.3 | |
| 2.58 | -1.00 | 1.49 | -1.00 | 16.06 | 294.56 | -28.20 | 62.91 | 0.5121 | -962.7 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 16.39 | 294.22 | -28.53 | 62.56 | 0.5184 | -572.0 | -427.3 | |
| 0.00 | 1.64 | 0.00 | 0.95 | 15.48 | 293.48 | -29.27 | 64.68 | 0.5234 | -739.0 | -493.8 | |
| 0.00 | 2.15 | 0.00 | 1.28 | 17.07 | 291.96 | -30.79 | 62.90 | 0.5518 | 754.0 | 594.3 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 15.97 | 292.16 | -30.60 | 64.65 | 0.5436 | 644.0 | 498.6 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 16.27 | 292.03 | -30.72 | 64.21 | 0.5468 | 482.0 | 363.2 | |
| 0.00 | 1.55 | 0.00 | 0.94 | 18.97 | 290.45 | -32.30 | 60.74 | 0.5815 | 847.0 | 573.4 | |
| 0.43 | 1.55 | 0.26 | 0.94 | 17.76 | 290.29 | -32.46 | 62.78 | 0.5770 | 671.4 | 499.2 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 18.37 | 290.09 | -32.66 | 61.91 | 0.5827 | 473.0 | 497.1 | |
| 0.00 | 1.72 | 0.00 | 1.07 | 20.56 | 289.48 | -33.27 | 58.88 | 0.6023 | -688.0 | -486.8 | |
| 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. | |