SDO HMI 2014-08-24 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.18 | 0.00 | 13.43 | -9.60 | 331.67 | 11.77 | 212.29 | 0.3668 | 114.7 | 147.7 | |
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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 |
| 0.00 | 0.81 | 0.00 | 0.48 | -9.20 | 348.44 | 28.54 | 240.72 | 0.5428 | 349.0 | 379.7 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -9.76 | 344.43 | 24.53 | 235.85 | 0.4964 | 605.0 | 469.4 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -7.57 | 339.46 | 19.56 | 233.61 | 0.4140 | 606.0 | 503.9 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -8.70 | 336.42 | 16.52 | 226.61 | 0.3884 | 721.0 | 657.7 | |
| 0.00 | 5.03 | 0.00 | 2.69 | -8.68 | 335.78 | 15.88 | 225.51 | 0.3808 | 920.0 | 699.5 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -8.45 | 335.64 | 15.74 | 225.69 | 0.3766 | 1012.0 | 903.3 | |
| 0.00 | 2.25 | 0.00 | 1.20 | -8.96 | 335.63 | 15.73 | 224.72 | 0.3822 | 833.0 | 740.2 | |
| 0.00 | 1.89 | 0.00 | 0.99 | -5.91 | 333.38 | 13.48 | 226.49 | 0.3211 | 951.0 | 780.6 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -13.74 | 332.26 | 12.36 | 210.62 | 0.4100 | -877.0 | -707.3 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -10.18 | 330.06 | 10.16 | 210.60 | 0.3426 | 768.0 | 634.6 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -13.29 | 328.85 | 8.95 | 203.66 | 0.3787 | -831.0 | -659.8 | |
| 0.00 | 1.98 | 0.00 | 1.06 | -13.45 | 328.63 | 8.73 | 202.99 | 0.3797 | -696.0 | -635.3 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -9.36 | 319.17 | -0.73 | 177.45 | 0.2832 | -906.0 | -692.4 | |
| 0.00 | 2.96 | 0.00 | 1.53 | -8.98 | 319.11 | -0.79 | 177.17 | 0.2769 | -1004.0 | -746.0 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -9.58 | 319.01 | -0.88 | 176.95 | 0.2871 | -731.0 | -573.8 | |
| 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. | |