SDO HMI 2014-01-11 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.91 | 23.36 | 2.13 | 12.81 | -17.93 | 28.99 | -21.69 | 124.61 | 0.4291 | 243.8 | 277.3 | |
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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 | 1.78 | 0.00 | 0.97 | -18.11 | 30.16 | -20.52 | 126.36 | 0.4155 | 947.0 | 693.4 | |
| 0.00 | 2.04 | 0.00 | 1.11 | -17.62 | 30.08 | -20.59 | 125.26 | 0.4123 | 798.0 | 670.3 | |
| 0.00 | 3.40 | 0.00 | 1.85 | -17.34 | 29.82 | -20.86 | 124.36 | 0.4135 | 730.0 | 804.3 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -18.85 | 29.40 | -21.28 | 126.92 | 0.4315 | 732.0 | 565.5 | |
| 3.91 | 7.31 | 2.13 | 3.99 | -17.45 | 29.21 | -21.47 | 123.88 | 0.4223 | 869.6 | 634.2 | |
| 0.00 | 0.76 | 0.00 | 0.42 | -19.20 | 28.47 | -22.20 | 126.52 | 0.4459 | 399.0 | 374.3 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -17.79 | 28.33 | -22.34 | 123.61 | 0.4365 | 770.0 | 502.7 | |
| 0.00 | 1.19 | 0.00 | 0.66 | -18.78 | 27.93 | -22.75 | 125.12 | 0.4495 | -893.0 | -654.4 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -19.05 | 27.62 | -23.06 | 125.30 | 0.4556 | -728.0 | -532.2 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -18.34 | 27.48 | -23.19 | 123.81 | 0.4518 | -774.0 | -607.8 | |
| 0.00 | 2.21 | 0.00 | 1.23 | -18.49 | 27.36 | -23.32 | 123.97 | 0.4546 | -876.0 | -790.1 | |
| 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. | |