SDO HMI 2014-11-04 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.47 | 0.00 | 9.07 | -21.44 | 76.90 | -18.79 | 146.48 | 0.5224 | 514.6 | 427.3 | |
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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 |
| 0.00 | 2.51 | 0.00 | 1.33 | -15.02 | 86.31 | -9.39 | 154.24 | 0.3643 | 752.0 | 620.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -20.88 | 83.12 | -12.57 | 154.19 | 0.4692 | 245.0 | 386.0 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -20.65 | 82.88 | -12.82 | 153.54 | 0.4677 | 526.0 | 517.2 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -20.62 | 82.66 | -13.04 | 153.11 | 0.4689 | 678.0 | 547.3 | |
| 0.00 | 1.90 | 0.00 | 1.07 | -19.98 | 79.90 | -15.80 | 147.75 | 0.4815 | 780.0 | 636.9 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -20.35 | 79.43 | -16.26 | 147.44 | 0.4899 | 607.0 | 596.9 | |
| 0.00 | 1.56 | 0.00 | 0.90 | -20.28 | 76.88 | -18.82 | 143.51 | 0.5109 | 740.0 | 562.8 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -22.79 | 76.50 | -19.20 | 145.95 | 0.5436 | 588.0 | 466.2 | |
| 0.00 | 1.56 | 0.00 | 0.90 | -20.49 | 76.32 | -19.38 | 142.98 | 0.5184 | 585.0 | 513.1 | |
| 0.00 | 1.90 | 0.00 | 1.22 | -25.54 | 68.87 | -26.82 | 140.14 | 0.6375 | 727.0 | 539.3 | |
| 0.00 | 1.64 | 0.00 | 1.15 | -28.34 | 63.21 | -32.49 | 138.08 | 0.7101 | -567.0 | -432.4 | |
| 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. | |