SDO HMI 2014-03-28 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.16 | 0.00 | 10.19 | -26.03 | 88.87 | -39.06 | 122.74 | 0.6603 | 231.2 | 166.8 | |
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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 | 1.14 | 0.00 | 0.64 | -22.47 | 102.68 | -25.24 | 125.57 | 0.4864 | 799.0 | 693.1 | |
| 0.00 | 2.19 | 0.00 | 1.25 | -23.10 | 101.43 | -26.49 | 125.56 | 0.5064 | 632.0 | 572.4 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -19.94 | 100.02 | -27.91 | 118.77 | 0.5040 | 684.0 | 496.7 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -22.06 | 99.54 | -28.38 | 122.22 | 0.5228 | 766.0 | 688.9 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -21.82 | 99.15 | -28.77 | 121.52 | 0.5262 | 668.0 | 529.6 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -26.69 | 89.80 | -38.13 | 123.41 | 0.6632 | 667.0 | 531.8 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -26.34 | 89.85 | -38.08 | 122.94 | 0.6609 | 354.0 | 423.1 | |
| 0.00 | 1.14 | 0.00 | 0.79 | -27.50 | 86.73 | -41.19 | 123.09 | 0.6995 | 587.0 | 506.5 | |
| 0.00 | 1.40 | 0.00 | 1.03 | -28.64 | 83.23 | -44.69 | 123.15 | 0.7395 | -671.0 | -574.7 | |
| 0.00 | 0.53 | 0.00 | 0.39 | -28.52 | 81.69 | -46.23 | 122.43 | 0.7541 | -468.0 | -407.0 | |
| 0.00 | 1.23 | 0.00 | 0.94 | -28.95 | 80.53 | -47.39 | 122.58 | 0.7665 | -380.0 | -352.6 | |
| 0.00 | 1.31 | 0.00 | 1.11 | -30.07 | 75.71 | -52.21 | 122.49 | 0.8131 | -274.0 | -215.6 | |
| 0.00 | 0.96 | 0.00 | 0.82 | -27.81 | 74.53 | -53.40 | 119.49 | 0.8180 | -358.0 | -285.6 | |
| 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. | |