SDO HMI 2014-04-24 01:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.73 | 0.00 | 7.94 | -12.45 | 140.32 | 0.57 | 177.35 | 0.1775 | 644.3 | 514.2 | |
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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 | 1.16 | 0.00 | 0.59 | -12.69 | 150.58 | 10.83 | 233.13 | 0.2302 | 717.0 | 579.4 | |
| 0.00 | 2.13 | 0.00 | 1.09 | -15.44 | 150.01 | 10.26 | 222.89 | 0.2534 | 698.0 | 585.4 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -13.83 | 149.68 | 9.93 | 226.87 | 0.2306 | 811.0 | 626.7 | |
| 0.00 | 1.07 | 0.00 | 0.53 | -9.10 | 145.58 | 5.83 | 233.48 | 0.1253 | 730.0 | 577.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -14.52 | 137.80 | -1.95 | 168.90 | 0.1717 | -878.0 | -699.6 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -15.44 | 137.04 | -2.71 | 166.06 | 0.1899 | 962.0 | 754.9 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -7.45 | 137.00 | -2.74 | 133.55 | 0.0658 | 685.0 | 429.4 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -15.25 | 136.85 | -2.89 | 164.89 | 0.1876 | 816.0 | 660.4 | |
| 0.00 | 1.07 | 0.00 | 0.53 | -10.02 | 136.58 | -3.17 | 148.81 | 0.1055 | 881.0 | 739.2 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -9.86 | 136.52 | -3.22 | 147.56 | 0.1038 | 775.0 | 680.6 | |
| 0.00 | 1.16 | 0.00 | 0.58 | -10.02 | 136.40 | -3.35 | 147.36 | 0.1072 | 779.0 | 608.5 | |
| 0.00 | 1.60 | 0.00 | 0.82 | -11.39 | 127.37 | -12.38 | 118.78 | 0.2408 | 756.0 | 528.7 | |
| 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. | |