SDO HMI 2014-01-12 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 25.78 | 0.23 | 14.06 | 16.57 | 25.15 | -13.46 | 31.97 | 0.4212 | 213.1 | 192.3 | |
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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 | 1.70 | 0.00 | 0.91 | 16.13 | 29.74 | -8.87 | 23.07 | 0.3797 | -904.0 | -750.0 | |
| 0.00 | 1.87 | 0.00 | 1.00 | 15.98 | 29.15 | -9.45 | 24.58 | 0.3813 | -836.0 | -643.0 | |
| 0.00 | 2.81 | 0.00 | 1.51 | 16.41 | 27.76 | -10.85 | 27.16 | 0.3973 | -832.0 | -815.0 | |
| 0.43 | 1.96 | 0.23 | 1.06 | 16.38 | 27.45 | -11.16 | 27.85 | 0.3992 | -940.2 | -770.7 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 17.48 | 26.31 | -12.30 | 28.84 | 0.4230 | -724.0 | -562.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 16.56 | 24.69 | -13.91 | 33.10 | 0.4239 | 905.0 | 757.6 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 16.95 | 24.22 | -14.39 | 33.45 | 0.4330 | 668.0 | 517.9 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 17.30 | 24.16 | -14.44 | 33.09 | 0.4380 | 817.0 | 687.7 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 16.63 | 24.02 | -14.58 | 34.23 | 0.4307 | 690.0 | 585.4 | |
| 0.00 | 1.87 | 0.00 | 1.03 | 17.27 | 23.84 | -14.76 | 33.69 | 0.4405 | 314.0 | 615.1 | |
| 0.00 | 2.38 | 0.00 | 1.30 | 15.94 | 23.91 | -14.69 | 35.39 | 0.4229 | 986.0 | 774.9 | |
| 0.00 | 2.55 | 0.00 | 1.39 | 15.82 | 23.67 | -14.94 | 36.00 | 0.4236 | 943.0 | 731.3 | |
| 0.00 | 2.47 | 0.00 | 1.37 | 17.29 | 22.78 | -15.82 | 35.50 | 0.4502 | 631.0 | 624.8 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 16.23 | 22.52 | -16.08 | 37.43 | 0.4394 | 909.0 | 763.1 | |
| 0.00 | 2.04 | 0.00 | 1.13 | 17.08 | 22.26 | -16.35 | 36.67 | 0.4524 | 835.0 | 666.0 | |
| 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. | |