SDO HMI 2014-10-05 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.23 | 32.14 | 3.64 | 18.46 | 12.46 | 91.12 | -29.83 | 76.35 | 0.5021 | -45.0 | 78.1 | |
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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 | 1.14 | 0.00 | 0.61 | 10.95 | 99.92 | -21.04 | 76.41 | 0.3642 | -835.0 | -647.6 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 11.21 | 98.88 | -22.08 | 76.21 | 0.3812 | -715.0 | -628.4 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 9.21 | 97.81 | -23.15 | 81.72 | 0.3938 | -665.0 | -547.9 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 10.31 | 96.73 | -24.23 | 79.29 | 0.4126 | -795.0 | -592.2 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 14.91 | 95.51 | -25.44 | 69.29 | 0.4457 | -507.0 | -359.4 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 10.26 | 95.69 | -25.26 | 79.69 | 0.4287 | -679.0 | -570.8 | |
| 0.00 | 2.02 | 0.00 | 1.11 | 10.97 | 95.36 | -25.60 | 78.15 | 0.4352 | -539.0 | -397.2 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 8.81 | 92.99 | -27.97 | 83.42 | 0.4684 | -690.0 | -454.3 | |
| 0.00 | 1.84 | 0.00 | 1.10 | 18.85 | 88.84 | -32.11 | 65.40 | 0.5555 | 692.0 | 510.0 | |
| 6.23 | 15.10 | 3.64 | 8.82 | 13.37 | 89.27 | -31.69 | 75.08 | 0.5310 | 1046.0 | 724.6 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 13.46 | 88.13 | -32.83 | 75.25 | 0.5474 | 728.0 | 564.1 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 18.59 | 86.01 | -34.95 | 67.14 | 0.5914 | 504.0 | 434.9 | |
| 0.00 | 1.84 | 0.00 | 1.10 | 7.30 | 87.11 | -33.85 | 86.57 | 0.5557 | -568.0 | -386.8 | |
| 0.00 | 0.97 | 0.00 | 0.59 | 8.54 | 84.84 | -36.12 | 84.39 | 0.5879 | -487.0 | -439.1 | |
| 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. | |