SDO HMI 2014-12-04 17:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.21 | 0.00 | 9.84 | 14.17 | 19.04 | -32.44 | 65.34 | 0.5738 | -591.8 | -469.2 | |
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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 | 1.37 | 0.00 | 0.76 | 11.21 | 26.66 | -24.82 | 65.53 | 0.4542 | -723.0 | -526.1 | |
| 0.00 | 1.19 | 0.00 | 0.69 | 15.33 | 24.09 | -27.39 | 59.86 | 0.5151 | -752.0 | -580.4 | |
| 0.00 | 1.88 | 0.00 | 1.10 | 13.77 | 22.19 | -29.29 | 64.04 | 0.5306 | -731.0 | -561.8 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 18.90 | 19.84 | -31.64 | 57.39 | 0.5914 | -679.0 | -554.7 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 16.67 | 19.73 | -31.75 | 60.91 | 0.5790 | -607.0 | -439.5 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 8.14 | 20.41 | -31.07 | 75.20 | 0.5305 | -808.0 | -670.2 | |
| 0.00 | 1.88 | 0.00 | 1.14 | 15.13 | 19.21 | -32.27 | 63.71 | 0.5771 | -713.0 | -496.1 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 13.54 | 17.76 | -33.72 | 67.11 | 0.5881 | -725.0 | -550.2 | |
| 0.00 | 1.02 | 0.00 | 0.64 | 15.49 | 16.86 | -34.62 | 64.52 | 0.6087 | -700.0 | -577.9 | |
| 0.00 | 1.96 | 0.00 | 1.21 | 13.78 | 16.91 | -34.57 | 67.17 | 0.6002 | -531.0 | -436.5 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 8.70 | 17.45 | -34.03 | 75.33 | 0.5741 | -747.0 | -611.2 | |
| 0.00 | 1.37 | 0.00 | 0.87 | 16.10 | 15.27 | -36.21 | 64.46 | 0.6314 | -594.0 | -499.3 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 18.28 | 9.69 | -41.79 | 64.04 | 0.7061 | 616.0 | 488.6 | |
| 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. | |