SDO HMI 2014-08-15 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.33 | 42.55 | 8.45 | 25.08 | -17.54 | 105.04 | 22.36 | 222.08 | 0.5433 | 395.0 | 371.6 | |
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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 | 0.99 | 0.00 | 0.59 | -17.53 | 106.17 | 23.49 | 223.51 | 0.5542 | 499.0 | 403.9 | |
| 1.26 | 4.51 | 0.75 | 2.68 | -17.58 | 105.94 | 23.25 | 223.15 | 0.5524 | 795.1 | 599.9 | |
| 5.41 | 12.99 | 3.20 | 7.67 | -17.21 | 105.82 | 23.14 | 223.49 | 0.5474 | 1016.4 | 775.2 | |
| 0.00 | 1.89 | 0.00 | 1.11 | -16.80 | 105.45 | 22.77 | 223.59 | 0.5395 | 675.0 | 529.6 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -17.62 | 105.42 | 22.74 | 222.47 | 0.5478 | 572.0 | 451.1 | |
| 0.00 | 1.35 | 0.00 | 0.82 | -20.16 | 105.68 | 23.00 | 219.67 | 0.5768 | 630.0 | 516.8 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -18.49 | 105.40 | 22.72 | 221.34 | 0.5566 | 777.0 | 698.7 | |
| 5.95 | 8.93 | 3.51 | 5.27 | -17.77 | 104.99 | 22.31 | 221.74 | 0.5451 | 934.6 | 692.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -16.52 | 103.78 | 21.10 | 221.80 | 0.5198 | -575.0 | -464.1 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -18.41 | 103.73 | 21.05 | 219.31 | 0.5401 | -574.0 | -496.2 | |
| 1.71 | 3.07 | 0.99 | 1.77 | -16.60 | 103.24 | 20.56 | 220.97 | 0.5154 | -847.9 | -649.9 | |
| 0.00 | 1.44 | 0.00 | 0.83 | -16.93 | 102.60 | 19.92 | 219.65 | 0.5129 | -921.0 | -621.4 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -20.50 | 102.77 | 20.09 | 215.58 | 0.5550 | 621.0 | 464.5 | |
| 0.00 | 1.80 | 0.00 | 1.04 | -17.81 | 102.09 | 19.41 | 217.82 | 0.5181 | -706.0 | -510.6 | |
| 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. | |