SDO HMI 2014-08-01 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.86 | 0.00 | 14.00 | 11.63 | 256.32 | -1.55 | 247.26 | 0.1402 | 784.4 | 634.2 | |
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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 | 1.36 | 0.00 | 0.69 | 15.73 | 268.13 | 10.26 | 315.30 | 0.2449 | -705.0 | -554.4 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 6.93 | 259.82 | 1.95 | 299.35 | 0.0390 | 931.0 | 635.6 | |
| 0.00 | 2.99 | 0.00 | 1.48 | 9.12 | 259.52 | 1.66 | 333.48 | 0.0643 | 955.0 | 706.4 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 16.14 | 258.69 | 0.83 | 355.57 | 0.1802 | 851.0 | 676.4 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 11.62 | 258.33 | 0.46 | 355.51 | 0.1016 | 897.0 | 671.6 | |
| 0.00 | 2.99 | 0.00 | 1.51 | 16.98 | 257.71 | -0.15 | 0.77 | 0.1940 | 811.0 | 667.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 18.31 | 257.58 | -0.28 | 1.24 | 0.2170 | 853.0 | 682.5 | |
| 0.00 | 2.71 | 0.00 | 1.37 | 15.89 | 257.55 | -0.31 | 1.72 | 0.1755 | 868.0 | 666.9 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 15.43 | 257.43 | -0.44 | 2.54 | 0.1675 | 820.0 | 628.1 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 4.01 | 256.24 | -1.63 | 138.35 | 0.0428 | 898.0 | 652.2 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 4.22 | 256.09 | -1.78 | 132.24 | 0.0420 | 967.0 | 840.7 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 4.07 | 255.97 | -1.90 | 132.92 | 0.0454 | 1107.0 | 861.3 | |
| 0.00 | 4.52 | 0.00 | 2.27 | 12.61 | 251.53 | -6.34 | 42.29 | 0.1609 | 930.0 | 695.6 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 1.67 | 251.57 | -6.29 | 123.34 | 0.1318 | 846.0 | 594.3 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 23.21 | 244.08 | -13.79 | 36.02 | 0.3741 | 737.0 | 533.4 | |
| 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. | |