SDO HMI 2014-11-14 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 | 18.58 | 0.00 | 9.85 | -9.90 | 337.27 | 16.16 | 230.83 | 0.3541 | -464.7 | -375.5 | |
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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 | 1.46 | 0.00 | 0.80 | -9.93 | 343.06 | 21.95 | 239.22 | 0.4303 | 787.0 | 571.8 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -10.27 | 341.95 | 20.84 | 237.21 | 0.4181 | 853.0 | 637.7 | |
| 0.00 | 1.46 | 0.00 | 0.79 | -10.92 | 341.03 | 19.92 | 234.70 | 0.4116 | 720.0 | 594.6 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -10.07 | 337.73 | 16.62 | 231.60 | 0.3610 | -857.0 | -711.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -9.73 | 337.46 | 16.35 | 231.90 | 0.3542 | -736.0 | -590.8 | |
| 0.00 | 1.55 | 0.00 | 0.82 | -9.55 | 337.39 | 16.28 | 232.20 | 0.3514 | -946.0 | -769.7 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -12.96 | 336.39 | 15.27 | 223.30 | 0.3760 | -779.0 | -591.8 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -9.67 | 335.56 | 14.45 | 228.57 | 0.3294 | -815.0 | -690.9 | |
| 0.00 | 2.24 | 0.00 | 1.17 | -9.27 | 335.17 | 14.06 | 228.75 | 0.3203 | -801.0 | -499.8 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -10.88 | 334.90 | 13.78 | 224.55 | 0.3350 | -798.0 | -629.2 | |
| 0.00 | 1.89 | 0.00 | 0.98 | -7.63 | 334.74 | 13.63 | 232.02 | 0.2976 | -868.0 | -685.8 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -9.05 | 334.70 | 13.58 | 228.31 | 0.3120 | -861.0 | -715.3 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -10.79 | 334.61 | 13.50 | 224.16 | 0.3306 | -940.0 | -728.9 | |
| 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. | |