SDO HMI 2014-11-04 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.15 | 40.05 | 6.93 | 21.38 | 5.53 | 71.77 | -21.74 | 85.13 | 0.3711 | -272.8 | -211.3 | |
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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 |
| 1.38 | 24.56 | 0.73 | 12.93 | 5.67 | 73.79 | -19.72 | 84.53 | 0.3387 | -1169.2 | -715.5 | |
| 8.13 | -1.00 | 4.28 | -1.00 | 5.88 | 73.69 | -19.82 | 83.94 | 0.3406 | -1108.1 | 999999 | |
| 3.29 | -1.00 | 1.73 | -1.00 | 5.70 | 73.60 | -19.91 | 84.49 | 0.3419 | -1077.1 | 999999 | |
| 0.00 | 3.03 | 0.00 | 1.60 | 5.16 | 73.43 | -20.08 | 86.10 | 0.3442 | -755.0 | -582.1 | |
| 0.00 | 1.47 | 0.00 | 0.78 | 5.44 | 72.84 | -20.66 | 85.36 | 0.3540 | -817.0 | -649.8 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 3.34 | 72.01 | -21.50 | 91.22 | 0.3675 | -823.0 | -635.8 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 4.77 | 71.97 | -21.54 | 87.32 | 0.3678 | -601.0 | -494.9 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 5.81 | 67.65 | -25.85 | 85.06 | 0.4373 | 718.0 | 533.8 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 5.95 | 67.41 | -26.09 | 84.77 | 0.4412 | 768.0 | 581.0 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 5.70 | 66.96 | -26.55 | 85.38 | 0.4481 | 908.0 | 779.5 | |
| 0.35 | 1.90 | 0.19 | 1.06 | 4.67 | 66.30 | -27.21 | 87.70 | 0.4580 | 924.8 | 792.7 | |
| 0.00 | 2.25 | 0.00 | 1.25 | 4.52 | 66.17 | -27.34 | 88.04 | 0.4600 | 937.0 | 794.0 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 5.10 | 64.79 | -28.71 | 86.82 | 0.4813 | 571.0 | 401.1 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 6.32 | 64.11 | -29.40 | 84.33 | 0.4923 | 562.0 | 474.3 | |
| 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. | |