SDO HMI 2014-11-02 16:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.19 | 0.00 | 8.19 | -19.93 | 78.45 | -35.41 | 126.22 | 0.6761 | 620.4 | 536.3 | |
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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 | 0.61 | 0.00 | 0.38 | -21.37 | 85.15 | -28.71 | 133.45 | 0.6184 | 647.0 | 565.4 | |
| 0.00 | 1.38 | 0.00 | 0.87 | -20.96 | 84.62 | -29.24 | 132.43 | 0.6202 | 738.0 | 557.8 | |
| 0.00 | 0.78 | 0.00 | 0.48 | -17.44 | 84.55 | -29.30 | 127.65 | 0.5920 | 530.0 | 494.6 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -20.00 | 79.18 | -34.68 | 126.68 | 0.6689 | 649.0 | 607.2 | |
| 0.00 | 1.04 | 0.00 | 0.70 | -20.51 | 78.07 | -35.78 | 126.52 | 0.6838 | 577.0 | 479.5 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -20.41 | 76.60 | -37.26 | 125.38 | 0.6982 | 588.0 | 468.3 | |
| 0.00 | 1.21 | 0.00 | 0.83 | -19.92 | 76.73 | -37.12 | 124.85 | 0.6937 | 624.0 | 627.5 | |
| 0.00 | 1.38 | 0.00 | 0.95 | -19.70 | 76.52 | -37.34 | 124.43 | 0.6947 | 654.0 | 560.9 | |
| 0.00 | 1.38 | 0.00 | 0.96 | -19.53 | 76.00 | -37.85 | 123.88 | 0.6989 | 640.0 | 527.6 | |
| 0.00 | 1.04 | 0.00 | 0.72 | -19.60 | 75.78 | -38.07 | 123.83 | 0.7017 | 665.0 | 581.8 | |
| 0.00 | 1.21 | 0.00 | 0.84 | -19.71 | 75.55 | -38.30 | 123.82 | 0.7047 | 512.0 | 410.6 | |
| 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. | |