SDO HMI 2014-10-04 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.07 | 0.00 | 10.43 | -17.65 | 103.43 | -31.83 | 128.78 | 0.6416 | -12.8 | -63.1 | |
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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 | 0.88 | 0.00 | 0.54 | -22.68 | 113.29 | -21.96 | 144.31 | 0.5938 | 697.0 | 630.1 | |
| 0.00 | 1.41 | 0.00 | 0.82 | -16.95 | 112.77 | -22.49 | 136.86 | 0.5371 | 733.0 | 585.1 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -17.17 | 112.37 | -22.89 | 136.64 | 0.5434 | 627.0 | 478.0 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -22.33 | 110.45 | -24.80 | 140.64 | 0.6142 | 383.0 | 375.2 | |
| 0.00 | 1.49 | 0.00 | 0.88 | -15.47 | 111.05 | -24.21 | 132.75 | 0.5402 | 753.0 | 596.8 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -17.00 | 108.45 | -26.81 | 131.95 | 0.5822 | 617.0 | 558.3 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -16.85 | 108.26 | -27.00 | 131.55 | 0.5828 | 798.0 | 680.8 | |
| 0.00 | 0.88 | 0.00 | 0.59 | -17.33 | 99.43 | -35.82 | 124.50 | 0.6803 | -666.0 | -564.4 | |
| 0.00 | 1.49 | 0.00 | 1.01 | -17.32 | 99.09 | -36.17 | 124.24 | 0.6839 | -680.0 | -569.2 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -17.52 | 98.92 | -36.34 | 124.39 | 0.6870 | -770.0 | -645.5 | |
| 0.00 | 1.85 | 0.00 | 1.26 | -17.47 | 98.70 | -36.56 | 124.17 | 0.6890 | -762.0 | -560.0 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -16.91 | 98.01 | -37.25 | 122.97 | 0.6927 | -571.0 | -482.0 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -17.01 | 97.51 | -37.75 | 122.76 | 0.6985 | -422.0 | -374.9 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -19.10 | 95.78 | -39.48 | 124.19 | 0.7287 | -463.0 | -389.2 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -16.38 | 95.44 | -39.81 | 120.66 | 0.7165 | -466.0 | -375.4 | |
| 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. | |