SDO HMI 2014-10-10 08:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.70 | 0.00 | 7.88 | 12.64 | 59.66 | -1.93 | 227.20 | 0.1561 | -153.4 | -108.5 | |
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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 | 1.58 | 0.00 | 0.80 | 16.92 | 68.60 | 7.01 | 327.98 | 0.2213 | -843.0 | -590.8 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.02 | 67.38 | 5.79 | 324.37 | 0.1689 | -840.0 | -636.7 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 11.34 | 63.71 | 2.12 | 338.00 | 0.0972 | -880.0 | -664.4 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 13.36 | 63.11 | 1.52 | 348.30 | 0.1280 | -823.0 | -620.2 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 14.18 | 62.99 | 1.40 | 350.29 | 0.1415 | -945.0 | -669.4 | |
| 0.00 | 1.49 | 0.00 | 0.75 | 14.48 | 62.78 | 1.19 | 352.05 | 0.1461 | -866.0 | -685.6 | |
| 0.00 | 1.32 | 0.00 | 0.65 | 10.27 | 62.08 | 0.50 | 353.14 | 0.0718 | -892.0 | -683.6 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 7.66 | 55.36 | -6.23 | 76.33 | 0.1111 | 867.0 | 671.1 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 13.52 | 55.22 | -6.37 | 40.12 | 0.1682 | 924.0 | 716.6 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 9.66 | 52.51 | -9.08 | 68.35 | 0.1681 | 725.0 | 567.9 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 14.49 | 51.10 | -10.49 | 50.40 | 0.2299 | 731.0 | 630.5 | |
| 0.00 | 1.40 | 0.00 | 0.71 | 10.74 | 50.56 | -11.02 | 66.65 | 0.2056 | 1001.0 | 757.1 | |
| 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. | |