SDO HMI 2014-12-08 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.74 | 0.00 | 9.98 | 15.13 | 18.88 | 14.09 | 318.51 | 0.3630 | -570.0 | -487.4 | |
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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 | 1.28 | 0.00 | 0.72 | 17.54 | 26.42 | 21.63 | 310.65 | 0.4653 | -681.0 | -545.1 | |
| 0.00 | 1.96 | 0.00 | 1.06 | 15.36 | 23.59 | 18.80 | 310.49 | 0.4103 | -820.0 | -588.0 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 12.47 | 22.51 | 17.72 | 306.04 | 0.3692 | -689.0 | -511.3 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 8.83 | 21.45 | 16.66 | 298.52 | 0.3238 | -780.0 | -665.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 12.89 | 21.59 | 16.80 | 308.42 | 0.3613 | -728.0 | -657.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 10.30 | 20.90 | 16.11 | 303.29 | 0.3280 | -728.0 | -585.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 16.90 | 21.12 | 16.33 | 317.26 | 0.3981 | -641.0 | -459.2 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 13.62 | 19.34 | 14.55 | 314.02 | 0.3410 | -803.0 | -496.8 | |
| 0.00 | 1.96 | 0.00 | 1.04 | 16.53 | 17.87 | 13.08 | 322.72 | 0.3597 | -857.0 | -783.3 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 12.62 | 17.63 | 12.84 | 315.28 | 0.3095 | -772.0 | -637.6 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 15.46 | 16.76 | 11.97 | 323.17 | 0.3349 | -886.0 | -717.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 15.46 | 16.54 | 11.75 | 323.67 | 0.3328 | -737.0 | -584.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 16.32 | 13.78 | 8.99 | 331.96 | 0.3203 | -787.0 | -521.1 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 19.96 | 9.76 | 4.97 | 346.60 | 0.3529 | 756.0 | 585.3 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 21.17 | 3.46 | -1.33 | 3.42 | 0.3637 | 603.0 | 418.0 | |
| 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. | |