SDO HMI 2014-09-06 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.81 | 0.00 | 10.91 | 10.35 | 177.97 | 23.22 | 284.13 | 0.4009 | -175.5 | 1.9 | |
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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 |
| 0.00 | 1.52 | 0.00 | 0.90 | 7.08 | 188.56 | 33.81 | 271.89 | 0.5546 | -594.0 | -528.9 | |
| 0.00 | 2.41 | 0.00 | 1.43 | 11.20 | 188.27 | 33.52 | 279.37 | 0.5512 | -285.0 | -305.3 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 10.92 | 187.43 | 32.67 | 278.96 | 0.5387 | -706.0 | -585.9 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 11.10 | 187.45 | 32.70 | 279.30 | 0.5392 | -642.0 | -565.8 | |
| 0.00 | 2.50 | 0.00 | 1.46 | 10.91 | 187.13 | 32.38 | 278.98 | 0.5345 | -716.0 | -607.7 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 11.53 | 187.03 | 32.28 | 280.15 | 0.5336 | -563.0 | -528.0 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 10.84 | 186.47 | 31.72 | 278.91 | 0.5247 | -707.0 | -649.3 | |
| 0.00 | 0.71 | 0.00 | 0.41 | 5.28 | 185.62 | 30.87 | 268.14 | 0.5132 | -545.0 | -477.4 | |
| 0.00 | 2.41 | 0.00 | 1.24 | 2.43 | 169.19 | 14.44 | 252.18 | 0.2628 | 885.0 | 642.5 | |
| 0.00 | 3.75 | 0.00 | 1.89 | 11.97 | 164.52 | 9.77 | 296.85 | 0.1869 | 1086.0 | 844.3 | |
| 0.00 | 2.86 | 0.00 | 1.44 | 16.02 | 161.33 | 6.58 | 324.27 | 0.1895 | 857.0 | 607.5 | |
| 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. | |