SDO HMI 2014-12-07 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.42 | 0.00 | 8.27 | -15.24 | 37.70 | 16.44 | 225.79 | 0.3821 | 208.7 | 20.8 | |
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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 |
| 0.00 | 0.77 | 0.00 | 0.42 | -17.51 | 41.23 | 19.98 | 227.05 | 0.4470 | 662.0 | 439.6 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -17.20 | 40.87 | 19.61 | 227.09 | 0.4397 | 767.0 | 595.0 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -19.82 | 40.81 | 19.56 | 222.69 | 0.4665 | 722.0 | 602.1 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -15.66 | 38.70 | 17.45 | 226.68 | 0.3986 | 865.0 | 697.7 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -15.81 | 38.71 | 17.46 | 226.41 | 0.4004 | 703.0 | 567.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -15.69 | 38.57 | 17.32 | 226.42 | 0.3974 | 889.0 | 753.7 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -15.07 | 37.63 | 16.37 | 226.04 | 0.3798 | 627.0 | 490.6 | |
| 0.00 | 3.41 | 0.00 | 1.80 | -13.12 | 36.04 | 14.78 | 227.29 | 0.3397 | -582.0 | -711.5 | |
| 0.00 | 1.79 | 0.00 | 0.94 | -13.33 | 35.74 | 14.48 | 226.24 | 0.3385 | -759.0 | -592.2 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -14.27 | 35.61 | 14.35 | 223.98 | 0.3476 | -776.0 | -635.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -15.03 | 34.74 | 13.49 | 220.71 | 0.3470 | -822.0 | -583.6 | |
| 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. | |