SDO HMI 2014-12-10 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.16 | 0.00 | 9.01 | 13.87 | 17.46 | 36.29 | 293.35 | 0.6284 | -494.6 | -442.1 | |
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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 | 2.22 | 0.00 | 1.49 | 13.23 | 21.91 | 40.74 | 290.06 | 0.6787 | -615.0 | -522.6 | |
| 0.00 | 1.70 | 0.00 | 1.12 | 9.85 | 21.23 | 40.06 | 285.36 | 0.6600 | -571.0 | -483.9 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 12.80 | 20.24 | 39.07 | 290.08 | 0.6568 | -616.0 | -587.7 | |
| 0.00 | 1.28 | 0.00 | 0.81 | 11.55 | 17.73 | 36.56 | 289.23 | 0.6204 | -696.0 | -615.6 | |
| 0.00 | 1.88 | 0.00 | 1.17 | 11.01 | 17.24 | 36.07 | 288.59 | 0.6120 | -587.0 | -519.6 | |
| 0.00 | 0.94 | 0.00 | 0.61 | 17.52 | 18.49 | 37.32 | 297.75 | 0.6556 | -504.0 | -417.5 | |
| 0.00 | 1.11 | 0.00 | 0.71 | 15.26 | 17.94 | 36.77 | 294.77 | 0.6384 | -599.0 | -535.7 | |
| 0.00 | 1.79 | 0.00 | 1.15 | 15.63 | 17.94 | 36.77 | 295.32 | 0.6401 | -581.0 | -527.5 | |
| 0.00 | 1.02 | 0.00 | 0.64 | 16.86 | 15.06 | 33.89 | 298.80 | 0.6113 | -691.0 | -560.9 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 12.94 | 12.92 | 31.75 | 293.91 | 0.5632 | -759.0 | -654.8 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 19.90 | 3.91 | 22.74 | 313.42 | 0.5025 | 778.0 | 648.9 | |
| 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. | |