SDO HMI 2014-04-22 14:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.41 | 0.00 | 8.78 | -19.94 | 125.66 | -33.38 | 117.71 | 0.5864 | 469.0 | 428.0 | |
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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 | 2.04 | 0.00 | 1.23 | -19.25 | 126.67 | -32.36 | 117.16 | 0.5701 | 477.0 | 517.5 | |
| 0.00 | 1.07 | 0.00 | 0.64 | -19.21 | 126.38 | -32.66 | 116.92 | 0.5737 | 717.0 | 615.8 | |
| 0.00 | 1.69 | 0.00 | 1.03 | -21.13 | 125.88 | -33.16 | 119.73 | 0.5897 | 580.0 | 418.1 | |
| 0.00 | 1.42 | 0.00 | 0.86 | -18.67 | 126.27 | -32.77 | 115.97 | 0.5725 | 659.0 | 545.9 | |
| 0.00 | 1.07 | 0.00 | 0.65 | -20.81 | 125.65 | -33.38 | 119.08 | 0.5908 | 606.0 | 556.6 | |
| 0.00 | 3.11 | 0.00 | 1.90 | -20.34 | 125.69 | -33.34 | 118.36 | 0.5879 | 774.0 | 468.8 | |
| 0.00 | 0.98 | 0.00 | 0.60 | -19.90 | 125.76 | -33.28 | 117.69 | 0.5849 | 608.0 | 485.1 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -20.42 | 125.48 | -33.56 | 118.37 | 0.5910 | 497.0 | 511.7 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -20.27 | 124.98 | -34.06 | 117.85 | 0.5965 | 662.0 | 533.1 | |
| 0.00 | 0.80 | 0.00 | 0.49 | -18.23 | 124.81 | -34.23 | 114.49 | 0.5893 | -747.0 | -617.6 | |
| 0.00 | 1.07 | 0.00 | 0.67 | -20.68 | 123.02 | -36.02 | 117.47 | 0.6224 | 326.0 | 313.2 | |
| 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. | |