SDO HMI 2014-08-25 23:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.03 | 0.00 | 8.40 | -10.35 | 329.70 | 29.09 | 238.82 | 0.5593 | -62.5 | -119.1 | |
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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 | 0.81 | 0.00 | 0.57 | -11.46 | 342.45 | 41.84 | 246.29 | 0.7163 | 622.0 | 483.9 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -9.76 | 337.12 | 36.51 | 245.62 | 0.6460 | 696.0 | 578.7 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -9.88 | 333.06 | 32.45 | 242.73 | 0.5969 | 610.0 | 502.9 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -10.63 | 332.52 | 31.91 | 241.19 | 0.5951 | -697.0 | -591.9 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -4.46 | 330.92 | 30.31 | 250.01 | 0.5375 | 780.0 | 559.8 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -9.50 | 331.21 | 30.60 | 241.89 | 0.5714 | 683.0 | 572.2 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -16.53 | 329.95 | 29.34 | 230.65 | 0.6096 | -692.0 | -541.5 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -10.02 | 325.11 | 24.50 | 235.29 | 0.4987 | -716.0 | -581.2 | |
| 0.00 | 2.15 | 0.00 | 1.23 | -9.94 | 324.86 | 24.26 | 235.15 | 0.4951 | -633.0 | -525.4 | |
| 0.00 | 1.53 | 0.00 | 0.89 | -12.95 | 325.00 | 24.39 | 230.53 | 0.5235 | -580.0 | -500.8 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -10.71 | 323.28 | 22.67 | 231.99 | 0.4826 | -761.0 | -599.8 | |
| 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. | |