SDO HMI 2014-10-10 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.00 | 0.00 | 9.60 | 14.32 | 58.30 | 4.97 | 288.00 | 0.1850 | -351.5 | -249.4 | |
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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 | 1.66 | 0.00 | 0.85 | 13.22 | 66.81 | 13.48 | 298.94 | 0.2604 | -696.0 | -681.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 16.51 | 63.39 | 10.05 | 317.22 | 0.2476 | -687.0 | -516.9 | |
| 0.00 | 2.36 | 0.00 | 1.21 | 18.20 | 60.68 | 7.35 | 329.85 | 0.2429 | -909.0 | -729.3 | |
| 0.00 | 1.40 | 0.00 | 0.71 | 14.74 | 60.54 | 7.21 | 320.94 | 0.1935 | -807.0 | -649.6 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 17.63 | 60.28 | 6.94 | 329.96 | 0.2312 | -914.0 | -734.0 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 16.84 | 60.12 | 6.79 | 328.65 | 0.2184 | -815.0 | -575.5 | |
| 0.00 | 1.84 | 0.00 | 0.92 | 12.71 | 58.87 | 5.54 | 320.46 | 0.1486 | 746.0 | 594.8 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 15.52 | 58.82 | 5.49 | 330.46 | 0.1878 | -890.0 | -729.0 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 15.85 | 58.64 | 5.31 | 332.13 | 0.1914 | -890.0 | -717.3 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 15.34 | 58.57 | 5.23 | 331.12 | 0.1830 | -807.0 | -647.6 | |
| 0.00 | 1.75 | 0.00 | 0.88 | 13.67 | 55.84 | 2.51 | 341.93 | 0.1377 | 843.0 | 716.5 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 13.37 | 54.58 | 1.24 | 350.43 | 0.1275 | 907.0 | 655.2 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 10.75 | 49.41 | -3.92 | 40.08 | 0.1048 | 693.0 | 515.5 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 6.96 | 47.72 | -5.61 | 81.74 | 0.0985 | -695.0 | -558.7 | |
| 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. | |