SDO HMI 2014-12-08 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.24 | 0.00 | 9.63 | 16.31 | 12.44 | 5.46 | 340.80 | 0.3420 | -149.9 | -181.0 | |
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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 | 1.36 | 0.00 | 0.76 | 20.42 | 25.58 | 18.61 | 319.39 | 0.4614 | -781.0 | -621.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 10.63 | 21.55 | 14.57 | 306.72 | 0.3098 | -812.0 | -636.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 10.39 | 20.27 | 13.29 | 308.57 | 0.2905 | -884.0 | -673.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 12.56 | 19.01 | 12.03 | 316.90 | 0.2991 | -803.0 | -658.1 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 17.64 | 18.71 | 11.73 | 327.40 | 0.3613 | -880.0 | -709.2 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 6.48 | 18.06 | 11.08 | 300.57 | 0.2228 | -863.0 | -699.5 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.56 | 17.79 | 10.82 | 327.74 | 0.3385 | -857.0 | -808.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 15.58 | 16.55 | 9.58 | 329.17 | 0.3141 | -813.0 | -680.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.93 | 9.68 | 2.71 | 352.58 | 0.3452 | 855.0 | 708.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 19.30 | 8.83 | 1.85 | 354.73 | 0.3334 | 808.0 | 642.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 20.66 | 5.28 | -1.70 | 4.50 | 0.3554 | 715.0 | 544.3 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 17.11 | 357.73 | -9.24 | 27.57 | 0.3333 | 737.0 | 554.0 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 20.36 | 355.25 | -11.73 | 28.72 | 0.3983 | 813.0 | 538.0 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 19.70 | 354.91 | -12.07 | 30.28 | 0.3919 | 667.0 | 517.9 | |
| 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. | |