SDO HMI 2014-11-06 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.53 | 22.96 | 4.21 | 17.37 | -15.72 | 16.12 | -45.54 | 114.66 | 0.7578 | -263.3 | -273.4 | |
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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 | 0.26 | 0.00 | 0.17 | -14.31 | 23.33 | -38.33 | 116.32 | 0.6728 | 512.0 | 467.3 | |
| 0.00 | 0.78 | 0.00 | 0.54 | -13.70 | 20.95 | -40.71 | 114.24 | 0.6973 | 506.0 | 418.1 | |
| 0.00 | 1.12 | 0.00 | 0.78 | -14.32 | 20.33 | -41.33 | 114.76 | 0.7071 | 590.0 | 508.5 | |
| 0.00 | 2.16 | 0.00 | 1.59 | -15.02 | 17.38 | -44.28 | 114.30 | 0.7422 | 586.0 | 514.4 | |
| 0.00 | 0.86 | 0.00 | 0.64 | -15.24 | 17.32 | -44.34 | 114.56 | 0.7438 | 355.0 | 354.0 | |
| 0.00 | 1.55 | 0.00 | 1.17 | -16.13 | 16.37 | -45.29 | 115.26 | 0.7572 | -820.0 | -693.9 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -16.84 | 16.02 | -45.64 | 115.99 | 0.7636 | -456.0 | -514.3 | |
| 0.00 | 0.78 | 0.00 | 0.59 | -16.24 | 16.12 | -45.54 | 115.29 | 0.7603 | -613.0 | -591.9 | |
| 3.54 | 9.32 | 2.69 | 7.06 | -15.87 | 16.01 | -45.66 | 114.78 | 0.7600 | -842.9 | -608.8 | |
| 1.99 | 3.97 | 1.52 | 3.04 | -16.05 | 15.55 | -46.11 | 114.81 | 0.7653 | -686.0 | -509.5 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -18.66 | 14.54 | -47.12 | 117.55 | 0.7854 | -358.0 | -352.0 | |
| 0.00 | 0.43 | 0.00 | 0.36 | -15.74 | 10.97 | -50.69 | 112.69 | 0.8094 | -572.0 | -527.8 | |
| 0.00 | 1.21 | 0.00 | 1.02 | -15.82 | 10.75 | -50.91 | 112.70 | 0.8117 | -425.0 | -369.5 | |
| 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. | |