SDO HMI 2014-08-11 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.94 | 99.39 | 30.95 | 158.00 | 14.07 | 55.00 | -72.85 | 77.26 | 0.9497 | -174.8 | 26.9 | |
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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 |
| 11.91 | 44.56 | 15.78 | 58.81 | 13.79 | 58.96 | -68.89 | 77.70 | 0.9288 | -554.1 | -295.9 | |
| 4.24 | 8.12 | 5.84 | 11.18 | 13.60 | 58.01 | -69.84 | 77.88 | 0.9348 | -358.9 | -165.6 | |
| 0.00 | 3.25 | 0.00 | 4.74 | 12.26 | 56.81 | -71.05 | 79.26 | 0.9421 | -539.0 | -421.9 | |
| 0.00 | 2.07 | 0.00 | 3.17 | 12.75 | 55.88 | -71.97 | 78.70 | 0.9472 | -148.0 | -117.9 | |
| 0.00 | 1.98 | 0.00 | 3.02 | 12.01 | 55.97 | -71.88 | 79.48 | 0.9469 | -290.0 | -194.1 | |
| 0.00 | 0.99 | 0.00 | 1.63 | 13.34 | 54.37 | -73.48 | 78.01 | 0.9550 | 73.0 | 61.4 | |
| 2.35 | 26.70 | 4.64 | 52.09 | 14.98 | 51.20 | -76.65 | 76.15 | 0.9692 | 434.4 | 307.4 | |
| 2.44 | -7.00 | 4.69 | -7.00 | 14.51 | 51.57 | -76.28 | 76.65 | 0.9677 | 347.6 | 999999 | |
| 0.00 | 5.14 | 0.00 | 9.65 | 14.03 | 52.07 | -75.78 | 77.17 | 0.9657 | 555.0 | 489.9 | |
| 0.00 | 3.52 | 0.00 | 7.54 | 15.41 | 49.94 | -77.91 | 75.64 | 0.9741 | 111.0 | 84.1 | |
| 0.00 | 1.62 | 0.00 | 3.42 | 14.38 | 50.31 | -77.54 | 76.72 | 0.9729 | 264.0 | 151.3 | |
| 0.00 | 1.44 | 0.00 | 2.75 | 12.48 | 51.84 | -76.01 | 78.77 | 0.9670 | 357.0 | 318.1 | |
| 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. | |