SDO HMI 2014-12-02 14:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.30 | 26.13 | 1.52 | 17.89 | -15.30 | 38.56 | -40.93 | 113.53 | 0.6907 | -37.5 | 128.9 | |
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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 |
| 1.45 | 8.63 | 0.94 | 5.58 | -16.51 | 42.82 | -36.67 | 117.16 | 0.6459 | 876.0 | 667.5 | |
| 0.00 | 0.60 | 0.00 | 0.40 | -16.22 | 40.02 | -39.47 | 115.31 | 0.6775 | 560.0 | 460.6 | |
| 0.00 | 0.51 | 0.00 | 0.35 | -15.61 | 39.00 | -40.49 | 113.99 | 0.6868 | 428.0 | 515.3 | |
| 0.00 | 1.62 | 0.00 | 1.11 | -15.96 | 38.71 | -40.77 | 114.33 | 0.6915 | 560.0 | 440.3 | |
| 0.85 | 3.67 | 0.58 | 2.49 | -15.15 | 38.83 | -40.66 | 113.27 | 0.6870 | 787.4 | 564.0 | |
| 0.00 | 0.94 | 0.00 | 0.64 | -14.42 | 38.51 | -40.98 | 112.12 | 0.6879 | 483.0 | 482.6 | |
| 0.00 | 1.88 | 0.00 | 1.33 | -14.62 | 36.23 | -43.26 | 111.50 | 0.7150 | -591.0 | -579.7 | |
| 0.00 | 1.20 | 0.00 | 0.85 | -14.87 | 36.13 | -43.36 | 111.79 | 0.7170 | -780.0 | -695.9 | |
| 0.00 | 0.68 | 0.00 | 0.49 | -15.12 | 35.85 | -43.64 | 112.02 | 0.7210 | -634.0 | -586.8 | |
| 0.00 | 1.37 | 0.00 | 0.97 | -14.93 | 35.73 | -43.76 | 111.73 | 0.7218 | -647.0 | -564.8 | |
| 0.00 | 1.45 | 0.00 | 1.06 | -15.99 | 34.88 | -44.60 | 112.81 | 0.7347 | -510.0 | -352.8 | |
| 0.00 | 1.02 | 0.00 | 0.75 | -14.43 | 34.36 | -45.13 | 110.57 | 0.7355 | -524.0 | -423.3 | |
| 0.00 | 1.79 | 0.00 | 1.32 | -13.70 | 33.72 | -45.77 | 109.40 | 0.7404 | -585.0 | -436.9 | |
| 0.00 | 0.77 | 0.00 | 0.55 | -9.40 | 33.85 | -45.64 | 103.69 | 0.7283 | 453.0 | 409.9 | |
| 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. | |