SDO HMI 2014-11-02 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 11.96 | 0.40 | 8.79 | -19.08 | 79.45 | -42.07 | 120.97 | 0.7385 | 552.7 | 448.2 | |
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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 | 1.13 | 0.00 | 0.72 | -14.82 | 86.75 | -34.77 | 119.71 | 0.6370 | 680.0 | 463.1 | |
| 0.00 | 1.04 | 0.00 | 0.71 | -20.93 | 84.85 | -36.67 | 126.48 | 0.6960 | 629.0 | 402.8 | |
| 0.00 | 0.52 | 0.00 | 0.35 | -17.73 | 84.75 | -36.77 | 122.33 | 0.6771 | 666.0 | 477.5 | |
| 0.00 | 1.30 | 0.00 | 0.87 | -16.97 | 84.58 | -36.94 | 121.22 | 0.6745 | 124.0 | 130.2 | |
| 0.00 | 0.87 | 0.00 | 0.63 | -19.86 | 79.97 | -41.56 | 122.12 | 0.7389 | 409.0 | 467.2 | |
| 0.00 | 0.78 | 0.00 | 0.58 | -19.94 | 78.57 | -42.95 | 121.44 | 0.7531 | 646.0 | 522.3 | |
| 0.00 | 0.78 | 0.00 | 0.61 | -20.56 | 76.71 | -44.81 | 121.22 | 0.7739 | 505.0 | 369.7 | |
| 0.52 | 2.34 | 0.40 | 1.81 | -19.79 | 76.55 | -44.97 | 120.22 | 0.7720 | 743.8 | 577.5 | |
| 0.00 | 0.43 | 0.00 | 0.34 | -19.50 | 76.43 | -45.10 | 119.83 | 0.7719 | 480.0 | 421.8 | |
| 0.00 | 0.78 | 0.00 | 0.61 | -19.64 | 76.33 | -45.19 | 119.94 | 0.7734 | 495.0 | 455.1 | |
| 0.00 | 0.95 | 0.00 | 0.74 | -19.25 | 76.38 | -45.14 | 119.50 | 0.7712 | 697.0 | 608.5 | |
| 0.00 | 1.04 | 0.00 | 0.82 | -19.38 | 75.66 | -45.87 | 119.32 | 0.7788 | 481.0 | 428.5 | |
| 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. | |