SDO HMI 2014-07-03 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.44 | 0.00 | 7.27 | -12.58 | 253.80 | -27.77 | 120.40 | 0.5286 | 337.9 | 283.9 | |
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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 | 0.73 | 0.00 | 0.41 | -13.40 | 258.67 | -22.90 | 126.57 | 0.4732 | 661.0 | 591.4 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -13.09 | 257.92 | -23.65 | 125.19 | 0.4800 | 492.0 | 416.7 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -11.99 | 257.59 | -23.99 | 122.86 | 0.4753 | 821.0 | 673.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -12.39 | 255.58 | -25.99 | 121.54 | 0.5042 | 752.0 | 594.7 | |
| 0.00 | 2.18 | 0.00 | 1.26 | -11.90 | 254.70 | -26.88 | 119.88 | 0.5122 | 590.0 | 510.9 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -14.52 | 252.77 | -28.80 | 122.51 | 0.5552 | 629.0 | 617.3 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -9.56 | 252.93 | -28.64 | 114.33 | 0.5208 | 649.0 | 451.2 | |
| 0.00 | 1.18 | 0.00 | 0.72 | -15.07 | 250.39 | -31.18 | 121.41 | 0.5880 | -500.0 | -418.5 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -9.90 | 251.01 | -30.56 | 113.57 | 0.5486 | 765.0 | 622.2 | |
| 0.00 | 1.18 | 0.00 | 0.72 | -15.24 | 250.17 | -31.40 | 121.49 | 0.5917 | -520.0 | -370.6 | |
| 0.00 | 0.82 | 0.00 | 0.50 | -13.43 | 248.79 | -32.78 | 117.75 | 0.5972 | -622.0 | -542.9 | |
| 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. | |