SDO HMI 2014-10-15 14:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.54 | 408.64 | 38.46 | 251.21 | -21.18 | 17.01 | 24.67 | 221.13 | 0.5942 | 948.7 | 340.6 | |
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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 | 1.57 | 0.00 | 0.93 | -17.12 | 16.86 | 24.52 | 226.14 | 0.5523 | -533.0 | -469.6 | |
| 32.84 | 396.58 | 20.26 | 243.91 | -21.22 | 17.42 | 25.08 | 221.54 | 0.5981 | 1112.1 | 354.2 | |
| 29.70 | -2.00 | 18.20 | -2.00 | -21.03 | 16.85 | 24.51 | 221.13 | 0.5909 | 1335.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -20.08 | 15.68 | 23.34 | 220.92 | 0.5703 | 622.0 | 547.0 | |
| 0.00 | 2.01 | 0.00 | 1.23 | -21.75 | 15.78 | 23.44 | 219.06 | 0.5886 | 77.0 | 116.0 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -23.51 | 15.71 | 23.37 | 217.01 | 0.6065 | 567.0 | 469.0 | |
| 0.00 | 1.66 | 0.00 | 1.01 | -22.31 | 14.55 | 22.20 | 216.96 | 0.5838 | 581.0 | 499.4 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -20.81 | 14.17 | 21.83 | 218.20 | 0.5642 | 559.0 | 447.4 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -22.74 | 9.82 | 17.48 | 210.31 | 0.5512 | -674.0 | -494.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -27.28 | 5.78 | 13.44 | 200.80 | 0.5840 | -707.0 | -587.2 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -28.93 | 3.92 | 11.58 | 197.18 | 0.5972 | -606.0 | -522.9 | |
| 0.00 | 1.22 | 0.00 | 0.75 | -28.42 | 3.83 | 11.49 | 197.34 | 0.5900 | -740.0 | -611.9 | |
| 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. | |