SDO HMI 2014-11-02 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.91 | 75.09 | 19.37 | 55.51 | 5.83 | 67.98 | -48.07 | 85.95 | 0.7437 | -170.6 | 279.9 | |
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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 |
| 4.33 | 15.66 | 2.98 | 10.78 | 5.84 | 71.92 | -44.13 | 85.98 | 0.6968 | -908.2 | -654.7 | |
| 3.37 | -1.00 | 2.32 | -1.00 | 6.02 | 71.90 | -44.15 | 85.72 | 0.6970 | -871.9 | 999999 | |
| 2.25 | -1.00 | 1.55 | -1.00 | 5.63 | 71.90 | -44.15 | 86.28 | 0.6970 | -786.2 | 999999 | |
| 1.30 | -1.00 | 0.90 | -1.00 | 6.13 | 71.81 | -44.25 | 85.56 | 0.6982 | -633.3 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 6.27 | 71.50 | -44.55 | 85.37 | 0.7020 | -481.0 | -342.5 | |
| 5.54 | 7.61 | 3.89 | 5.34 | 5.60 | 70.80 | -45.25 | 86.31 | 0.7106 | -517.3 | -357.7 | |
| 0.00 | 2.34 | 0.00 | 1.68 | 6.25 | 69.48 | -46.57 | 85.40 | 0.7266 | -554.0 | -436.3 | |
| 0.00 | 1.64 | 0.00 | 1.20 | 6.53 | 68.52 | -47.53 | 85.02 | 0.7379 | -351.0 | -270.7 | |
| 0.69 | 1.90 | 0.51 | 1.40 | 5.07 | 68.10 | -47.95 | 86.99 | 0.7430 | -352.4 | -320.9 | |
| 1.73 | 7.44 | 1.31 | 5.63 | 6.80 | 66.90 | -49.15 | 84.67 | 0.7567 | 782.8 | 585.8 | |
| 0.00 | 1.56 | 0.00 | 1.18 | 5.82 | 66.47 | -49.58 | 85.96 | 0.7616 | 746.0 | 692.6 | |
| 1.99 | 15.14 | 1.52 | 11.58 | 6.14 | 66.30 | -49.76 | 85.54 | 0.7636 | 687.0 | 614.7 | |
| 0.43 | -12.00 | 0.33 | -12.00 | 5.82 | 65.96 | -50.09 | 85.95 | 0.7673 | 365.8 | 999999 | |
| 5.28 | 21.11 | 4.06 | 16.24 | 5.37 | 65.92 | -50.13 | 86.54 | 0.7679 | 649.5 | 394.9 | |
| 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. | |