SDO HMI 2014-09-07 11:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.96 | 36.32 | 12.52 | 39.34 | -20.88 | 78.32 | -57.19 | 118.03 | 0.8899 | 4.3 | -64.7 | |
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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 |
| 0.98 | 2.77 | 0.95 | 2.67 | -20.57 | 82.51 | -53.00 | 119.30 | 0.8594 | 608.5 | 487.9 | |
| 0.89 | 1.70 | 0.87 | 1.65 | -20.26 | 81.96 | -53.55 | 118.74 | 0.8626 | 473.9 | 415.8 | |
| 1.07 | 2.59 | 1.05 | 2.54 | -20.48 | 81.80 | -53.71 | 118.90 | 0.8646 | 348.4 | 271.0 | |
| 0.00 | 1.25 | 0.00 | 1.26 | -21.26 | 81.04 | -54.47 | 119.44 | 0.8728 | 411.0 | 370.4 | |
| 0.36 | 1.61 | 0.37 | 1.66 | -21.43 | 80.10 | -55.42 | 119.25 | 0.8802 | 583.5 | 495.6 | |
| 0.00 | 0.89 | 0.00 | 0.94 | -21.58 | 79.72 | -55.79 | 119.25 | 0.8833 | 159.0 | 122.2 | |
| 3.30 | 5.00 | 3.42 | 5.17 | -21.08 | 79.95 | -55.56 | 118.81 | 0.8802 | 355.4 | 193.5 | |
| 0.00 | 0.89 | 0.00 | 0.93 | -19.80 | 79.10 | -56.41 | 117.13 | 0.8826 | -558.0 | -466.5 | |
| 0.00 | 0.71 | 0.00 | 0.75 | -20.05 | 78.96 | -56.55 | 117.34 | 0.8843 | -449.0 | -451.9 | |
| 4.91 | 13.92 | 5.28 | 14.93 | -20.03 | 78.20 | -57.31 | 117.05 | 0.8897 | -478.6 | -381.6 | |
| 0.45 | 2.05 | 0.58 | 2.66 | -22.45 | 73.46 | -62.05 | 117.97 | 0.9259 | 284.4 | 208.0 | |
| 0.00 | 1.87 | 0.00 | 2.63 | -23.33 | 71.78 | -63.73 | 118.34 | 0.9370 | -133.0 | -150.6 | |
| 0.00 | 1.07 | 0.00 | 1.55 | -23.13 | 70.90 | -64.61 | 117.87 | 0.9413 | -356.0 | -286.2 | |
| 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. | |