SDO HMI 2014-11-03 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.75 | 0.00 | 11.11 | -20.10 | 78.67 | -29.12 | 131.59 | 0.6117 | 713.8 | 585.7 | |
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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 | 2.68 | 0.00 | 1.60 | -20.99 | 85.04 | -22.75 | 139.32 | 0.5561 | 785.0 | 639.9 | |
| 0.00 | 0.87 | 0.00 | 0.50 | -16.66 | 84.95 | -22.84 | 133.31 | 0.5130 | 824.0 | 740.4 | |
| 0.00 | 2.08 | 0.00 | 1.29 | -20.05 | 79.53 | -28.25 | 132.14 | 0.6020 | 817.0 | 604.5 | |
| 0.00 | 1.30 | 0.00 | 0.81 | -20.45 | 78.47 | -29.31 | 131.66 | 0.6163 | 769.0 | 668.1 | |
| 0.00 | 1.56 | 0.00 | 0.98 | -20.55 | 78.45 | -29.33 | 131.77 | 0.6173 | 549.0 | 517.9 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -19.99 | 76.88 | -30.90 | 129.64 | 0.6290 | 673.0 | 599.5 | |
| 0.00 | 1.73 | 0.00 | 1.11 | -20.39 | 76.61 | -31.18 | 129.92 | 0.6350 | 741.0 | 602.5 | |
| 0.00 | 2.51 | 0.00 | 1.61 | -20.17 | 76.40 | -31.39 | 129.46 | 0.6355 | 762.0 | 535.8 | |
| 0.00 | 0.61 | 0.00 | 0.39 | -19.91 | 76.31 | -31.48 | 129.05 | 0.6345 | 790.0 | 594.0 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -19.82 | 76.14 | -31.64 | 128.79 | 0.6355 | 725.0 | 575.2 | |
| 0.00 | 0.52 | 0.00 | 0.33 | -19.80 | 75.92 | -31.86 | 128.58 | 0.6376 | 588.0 | 422.8 | |
| 0.00 | 1.64 | 0.00 | 1.06 | -19.75 | 75.56 | -32.22 | 128.21 | 0.6411 | 542.0 | 510.8 | |
| 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. | |