SDO HMI 2014-11-02 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.35 | 0.00 | 8.31 | -20.04 | 77.50 | -35.25 | 126.58 | 0.6739 | 497.2 | 430.6 | |
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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 | 1.64 | 0.00 | 1.02 | -21.24 | 84.95 | -27.80 | 134.15 | 0.6082 | 667.0 | 539.4 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -17.40 | 84.49 | -28.26 | 128.57 | 0.5800 | 504.0 | 436.1 | |
| 0.00 | 0.78 | 0.00 | 0.51 | -20.02 | 79.22 | -33.53 | 127.57 | 0.6571 | 683.0 | 606.1 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -20.32 | 76.71 | -36.04 | 126.10 | 0.6852 | 538.0 | 484.8 | |
| 0.00 | 0.69 | 0.00 | 0.47 | -20.00 | 76.72 | -36.03 | 125.69 | 0.6830 | 748.0 | 676.5 | |
| 0.00 | 0.95 | 0.00 | 0.65 | -20.43 | 76.56 | -36.19 | 126.13 | 0.6874 | 467.0 | 360.6 | |
| 0.00 | 2.33 | 0.00 | 1.59 | -19.60 | 76.12 | -36.63 | 124.78 | 0.6867 | 472.0 | 458.3 | |
| 0.00 | 1.12 | 0.00 | 0.76 | -19.45 | 75.96 | -36.79 | 124.48 | 0.6874 | 571.0 | 446.5 | |
| 0.00 | 1.12 | 0.00 | 0.77 | -19.65 | 75.83 | -36.92 | 124.64 | 0.6900 | 768.0 | 611.8 | |
| 0.00 | 1.30 | 0.00 | 0.89 | -19.72 | 75.57 | -37.18 | 124.56 | 0.6932 | 580.0 | 454.4 | |
| 0.00 | 0.69 | 0.00 | 0.58 | -24.18 | 65.72 | -47.04 | 124.24 | 0.8098 | -529.0 | -437.1 | |
| 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. | |