SDO HMI 2014-11-10 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.41 | 0.00 | 12.56 | -23.81 | 8.71 | -5.14 | 169.96 | 0.4666 | 669.1 | 576.2 | |
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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 | 0.26 | 0.00 | 0.14 | -20.74 | 10.23 | -3.62 | 171.78 | 0.4150 | 836.0 | 805.3 | |
| 0.00 | 2.41 | 0.00 | 1.32 | -21.29 | 10.18 | -3.67 | 171.88 | 0.4238 | 855.0 | 691.2 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -20.48 | 10.01 | -3.84 | 171.20 | 0.4114 | 660.0 | 574.5 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -23.57 | 9.47 | -4.38 | 171.23 | 0.4608 | 884.0 | 750.2 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -22.71 | 9.43 | -4.42 | 170.83 | 0.4476 | 825.0 | 671.8 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -23.87 | 9.10 | -4.75 | 170.62 | 0.4664 | 801.0 | 645.0 | |
| 0.00 | 3.28 | 0.00 | 1.85 | -24.78 | 9.00 | -4.85 | 170.77 | 0.4804 | 736.0 | 625.7 | |
| 0.00 | 3.53 | 0.00 | 1.99 | -24.45 | 8.98 | -4.87 | 170.60 | 0.4754 | 869.0 | 748.0 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -24.28 | 8.82 | -5.03 | 170.24 | 0.4732 | 936.0 | 719.5 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -23.98 | 8.70 | -5.14 | 169.90 | 0.4690 | 653.0 | 611.1 | |
| 0.00 | 1.98 | 0.00 | 1.13 | -25.33 | 8.55 | -5.30 | 170.14 | 0.4897 | 670.0 | 525.1 | |
| 0.00 | 2.33 | 0.00 | 1.31 | -24.08 | 8.31 | -5.54 | 169.18 | 0.4716 | 711.0 | 659.6 | |
| 0.00 | 1.47 | 0.00 | 0.85 | -26.29 | 2.77 | -11.07 | 160.80 | 0.5257 | -738.0 | -625.3 | |
| 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. | |