SDO HMI 2014-11-02 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.17 | 0.00 | 8.10 | -19.83 | 78.62 | -34.68 | 126.62 | 0.6677 | 590.7 | 474.8 | |
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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 | 1.12 | 0.00 | 0.70 | -20.97 | 84.61 | -28.69 | 132.96 | 0.6148 | 742.0 | 618.5 | |
| 0.00 | 1.12 | 0.00 | 0.69 | -17.60 | 84.66 | -28.65 | 128.49 | 0.5861 | 469.0 | 444.4 | |
| 0.00 | 1.90 | 0.00 | 1.23 | -20.53 | 81.54 | -31.76 | 129.65 | 0.6426 | 80.0 | 147.1 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -20.04 | 79.20 | -34.10 | 127.16 | 0.6633 | 738.0 | 592.1 | |
| 0.00 | 1.38 | 0.00 | 0.94 | -19.96 | 76.73 | -36.57 | 125.27 | 0.6883 | 688.0 | 574.9 | |
| 0.00 | 0.86 | 0.00 | 0.59 | -20.42 | 76.56 | -36.74 | 125.74 | 0.6930 | 652.0 | 488.2 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -19.74 | 76.55 | -36.75 | 124.87 | 0.6888 | 673.0 | 500.9 | |
| 0.00 | 1.04 | 0.00 | 0.71 | -19.57 | 76.01 | -37.30 | 124.29 | 0.6934 | 710.0 | 577.6 | |
| 0.00 | 1.38 | 0.00 | 0.95 | -19.61 | 75.80 | -37.51 | 124.21 | 0.6959 | 753.0 | 602.1 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -19.48 | 75.75 | -37.55 | 124.02 | 0.6956 | 425.0 | 430.3 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -19.72 | 75.57 | -37.74 | 124.19 | 0.6989 | 568.0 | 439.2 | |
| 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. | |