SDO HMI 2014-07-20 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.39 | 160.93 | 22.87 | 89.05 | -21.50 | 68.01 | 1.48 | 183.14 | 0.4465 | 193.4 | 106.4 | |
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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 |
| 15.16 | 93.94 | 8.38 | 51.93 | -21.42 | 69.45 | 2.92 | 186.12 | 0.4462 | 1126.6 | 405.5 | |
| 4.63 | -1.00 | 2.55 | -1.00 | -21.15 | 69.02 | 2.49 | 185.28 | 0.4412 | 932.6 | 999999 | |
| 4.18 | 12.25 | 2.29 | 6.74 | -20.77 | 68.49 | 1.96 | 184.23 | 0.4347 | 1120.3 | 772.2 | |
| 0.54 | 2.36 | 0.30 | 1.30 | -20.80 | 68.10 | 1.57 | 183.39 | 0.4348 | 788.3 | 578.0 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.30 | 67.80 | 1.27 | 182.81 | 0.4265 | 777.0 | 562.8 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -21.11 | 67.74 | 1.21 | 182.58 | 0.4392 | -184.0 | -102.0 | |
| 2.45 | 14.89 | 1.35 | 8.23 | -21.34 | 65.94 | -0.59 | 178.76 | 0.4426 | -876.0 | -678.9 | |
| 7.44 | -7.00 | 4.12 | -7.00 | -21.58 | 65.81 | -0.72 | 178.50 | 0.4464 | -1021.8 | 999999 | |
| 0.00 | 2.81 | 0.00 | 1.56 | -21.78 | 65.55 | -0.98 | 177.96 | 0.4497 | -1077.0 | -895.1 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -22.64 | 65.44 | -1.09 | 177.82 | 0.4631 | -491.0 | -419.6 | |
| 1.45 | 31.59 | 0.81 | 17.58 | -22.26 | 65.38 | -1.15 | 177.66 | 0.4573 | -959.3 | -750.1 | |
| 1.00 | -11.00 | 0.55 | -11.00 | -22.02 | 65.22 | -1.31 | 177.30 | 0.4537 | -1061.8 | 999999 | |
| 4.54 | -11.00 | 2.52 | -11.00 | -22.23 | 65.12 | -1.41 | 177.12 | 0.4569 | -908.9 | 999999 | |
| 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. | |