SDO HMI 2014-10-12 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.56 | 0.00 | 12.78 | -22.44 | 69.29 | 33.54 | 227.73 | 0.6950 | -105.3 | -173.7 | |
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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 | 0.88 | 0.00 | 0.64 | -16.80 | 77.17 | 41.42 | 240.16 | 0.7325 | 236.0 | 390.0 | |
| 0.00 | 0.96 | 0.00 | 0.71 | -18.62 | 77.23 | 41.48 | 237.97 | 0.7427 | 214.0 | 338.2 | |
| 0.00 | 0.88 | 0.00 | 0.63 | -16.75 | 76.45 | 40.70 | 239.81 | 0.7248 | 508.0 | 478.5 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -18.38 | 75.65 | 39.90 | 237.32 | 0.7256 | 454.0 | 387.6 | |
| 0.00 | 0.96 | 0.00 | 0.69 | -19.75 | 75.14 | 39.39 | 235.34 | 0.7285 | 135.0 | 210.1 | |
| 0.00 | 1.31 | 0.00 | 0.93 | -22.73 | 71.88 | 36.13 | 229.58 | 0.7166 | 433.0 | 468.8 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -24.50 | 72.25 | 36.50 | 227.85 | 0.7323 | 266.0 | 316.4 | |
| 0.00 | 1.14 | 0.00 | 0.72 | -14.52 | 68.62 | 32.88 | 237.45 | 0.6256 | 338.0 | 340.4 | |
| 0.00 | 1.84 | 0.00 | 1.25 | -23.41 | 68.13 | 32.38 | 225.85 | 0.6873 | -733.0 | -649.5 | |
| 0.00 | 2.10 | 0.00 | 1.43 | -23.58 | 68.14 | 32.39 | 225.66 | 0.6887 | -708.0 | -577.7 | |
| 0.00 | 0.88 | 0.00 | 0.60 | -24.23 | 68.01 | 32.26 | 224.83 | 0.6927 | -544.0 | -515.8 | |
| 0.00 | 2.01 | 0.00 | 1.37 | -24.11 | 67.74 | 31.99 | 224.74 | 0.6894 | -583.0 | -518.0 | |
| 0.00 | 2.01 | 0.00 | 1.37 | -24.08 | 67.39 | 31.64 | 224.46 | 0.6861 | -685.0 | -536.9 | |
| 0.00 | 1.40 | 0.00 | 0.95 | -29.68 | 60.61 | 24.87 | 212.40 | 0.6842 | -461.0 | -432.9 | |
| 0.00 | 1.14 | 0.00 | 0.73 | -26.46 | 58.27 | 22.52 | 212.87 | 0.6340 | -450.0 | -411.5 | |
| 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. | |