SDO HMI 2014-05-13 20:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.00 | 93.73 | 39.62 | 92.21 | 10.48 | 179.65 | -58.51 | 76.13 | 0.8654 | 96.3 | 157.9 | |
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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 |
| 15.61 | 47.26 | 14.75 | 44.84 | 9.99 | 180.94 | -57.22 | 76.45 | 0.8538 | -529.5 | 57.2 | |
| 4.30 | -1.00 | 4.08 | -1.00 | 9.63 | 180.75 | -57.41 | 76.90 | 0.8549 | -267.5 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.95 | 9.87 | 180.10 | -58.06 | 76.74 | 0.8609 | 335.0 | 315.3 | |
| 0.00 | 5.02 | 0.00 | 4.93 | 10.82 | 179.70 | -58.45 | 75.73 | 0.8657 | 534.0 | 331.4 | |
| 0.00 | 0.81 | 0.00 | 0.80 | 11.14 | 179.54 | -58.61 | 75.40 | 0.8676 | 213.0 | 158.2 | |
| 0.00 | 1.26 | 0.00 | 1.23 | 10.22 | 179.82 | -58.33 | 76.39 | 0.8638 | 282.0 | 243.9 | |
| 0.00 | 1.43 | 0.00 | 1.45 | 11.13 | 178.94 | -59.22 | 75.52 | 0.8726 | 481.0 | 414.9 | |
| 0.00 | 1.26 | 0.00 | 1.25 | 10.06 | 179.27 | -58.88 | 76.67 | 0.8682 | 222.0 | 170.8 | |
| 0.00 | 0.81 | 0.00 | 0.80 | 10.25 | 179.16 | -59.00 | 76.48 | 0.8695 | 204.0 | 175.8 | |
| 0.00 | 1.79 | 0.00 | 1.80 | 9.77 | 178.75 | -59.40 | 77.09 | 0.8722 | -276.0 | -162.9 | |
| 0.00 | 1.08 | 0.00 | 1.08 | 9.46 | 178.78 | -59.37 | 77.44 | 0.8716 | -438.0 | -238.1 | |
| 20.09 | 29.51 | 20.79 | 30.49 | 11.36 | 178.06 | -60.09 | 75.43 | 0.8800 | 579.2 | 395.0 | |
| 0.00 | 1.52 | 0.00 | 1.55 | 10.07 | 178.42 | -59.73 | 76.82 | 0.8754 | -123.0 | -53.1 | |
| 0.00 | 0.99 | 0.00 | 1.04 | 10.83 | 177.43 | -60.73 | 76.14 | 0.8844 | 299.0 | 290.5 | |
| 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. | |