SDO HMI 2014-09-19 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.32 | 228.59 | 35.77 | 176.08 | 8.25 | 290.04 | -50.31 | 85.21 | 0.7668 | -672.7 | -253.5 | |
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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 | 0.98 | 0.00 | 0.68 | 9.07 | 295.52 | -44.83 | 84.31 | 0.7020 | -594.0 | -500.5 | |
| 0.00 | 1.51 | 0.00 | 1.09 | 10.88 | 293.25 | -47.10 | 81.76 | 0.7293 | -626.0 | -468.7 | |
| 0.00 | 0.98 | 0.00 | 0.72 | 12.17 | 292.32 | -48.03 | 80.02 | 0.7403 | -481.0 | -403.5 | |
| 18.28 | 87.14 | 13.85 | 66.09 | 5.29 | 290.91 | -49.44 | 89.16 | 0.7589 | -844.3 | -271.8 | |
| 12.51 | 129.82 | 9.62 | 100.44 | 10.36 | 289.95 | -50.41 | 82.44 | 0.7669 | -1120.0 | -263.1 | |
| 0.00 | 1.06 | 0.00 | 0.81 | 5.77 | 290.48 | -49.87 | 88.49 | 0.7633 | 64.0 | 31.2 | |
| 10.38 | -5.00 | 8.04 | -5.00 | 10.27 | 289.58 | -50.77 | 82.56 | 0.7710 | -773.3 | 999999 | |
| 2.84 | -5.00 | 2.21 | -5.00 | 10.46 | 289.34 | -51.01 | 82.31 | 0.7736 | -625.3 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 5.64 | 288.23 | -52.13 | 88.42 | 0.7881 | 583.0 | 548.7 | |
| 0.00 | 1.24 | 0.00 | 1.08 | 6.46 | 284.85 | -55.50 | 87.09 | 0.8221 | 473.0 | 397.9 | |
| 0.00 | 0.98 | 0.00 | 0.86 | 4.42 | 284.54 | -55.81 | 89.52 | 0.8269 | -81.0 | -107.3 | |
| 0.00 | 0.44 | 0.00 | 0.39 | 5.46 | 284.25 | -56.11 | 88.24 | 0.8289 | 372.0 | 312.4 | |
| 2.31 | 4.17 | 2.05 | 3.71 | 5.29 | 283.83 | -56.52 | 88.40 | 0.8330 | 445.2 | 222.3 | |
| 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. | |