SDO HMI 2014-11-29 22:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.28 | 18.37 | 0.74 | 10.79 | -23.02 | 92.40 | -22.20 | 139.50 | 0.5378 | -254.5 | -220.2 | |
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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 | 1.79 | 0.00 | 1.01 | -21.97 | 97.16 | -17.45 | 144.54 | 0.4814 | 516.0 | 439.8 | |
| 0.00 | 1.79 | 0.00 | 1.04 | -23.60 | 94.82 | -19.78 | 143.31 | 0.5212 | 857.0 | 653.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -20.74 | 94.57 | -20.03 | 139.13 | 0.4917 | -464.0 | -486.7 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -23.84 | 92.71 | -21.90 | 140.91 | 0.5432 | -839.0 | -628.6 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -24.01 | 92.43 | -22.17 | 140.78 | 0.5475 | -729.0 | -684.4 | |
| 0.00 | 0.94 | 0.00 | 0.56 | -24.17 | 92.37 | -22.24 | 140.91 | 0.5498 | -770.0 | -579.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | -24.08 | 92.10 | -22.50 | 140.48 | 0.5512 | -618.0 | -553.2 | |
| 0.00 | 1.28 | 0.00 | 0.78 | -25.50 | 90.76 | -23.85 | 140.69 | 0.5783 | -728.0 | -589.5 | |
| 0.00 | 1.03 | 0.00 | 0.62 | -25.30 | 90.58 | -24.02 | 140.26 | 0.5779 | -769.0 | -625.0 | |
| 1.28 | 2.48 | 0.74 | 1.43 | -19.96 | 91.39 | -23.21 | 133.97 | 0.5168 | -661.9 | -495.0 | |
| 0.00 | 2.14 | 0.00 | 1.30 | -25.17 | 90.25 | -24.35 | 139.73 | 0.5796 | -796.0 | -567.4 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -19.90 | 90.89 | -23.72 | 133.29 | 0.5217 | 738.0 | 599.6 | |
| 0.00 | 1.11 | 0.00 | 0.65 | -20.45 | 90.42 | -24.19 | 133.56 | 0.5319 | 849.0 | 709.5 | |
| 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. | |