SDO HMI 2014-05-26 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.57 | 179.50 | 96.55 | 439.27 | -18.76 | 150.14 | 77.89 | 251.05 | 0.9772 | 25.1 | -39.9 | |
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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 |
| 0.00 | 2.16 | 0.00 | 6.37 | -17.39 | 152.44 | 80.19 | 252.58 | 0.9863 | 267.0 | 231.5 | |
| 12.36 | 68.64 | 41.93 | 239.13 | -18.45 | 153.79 | 81.54 | 251.55 | 0.9898 | 42.8 | -49.3 | |
| 1.17 | 7.76 | 2.60 | 17.28 | -17.56 | 149.10 | 76.85 | 252.29 | 0.9756 | -161.3 | 270.5 | |
| 0.00 | 1.89 | 0.00 | 4.88 | -18.99 | 151.02 | 78.76 | 250.91 | 0.9823 | 283.0 | 232.9 | |
| 2.71 | 27.15 | 4.82 | 48.04 | -17.44 | 145.78 | 73.53 | 252.23 | 0.9619 | -323.7 | -254.6 | |
| 3.07 | -5.00 | 5.40 | -5.00 | -17.73 | 145.53 | 73.27 | 251.91 | 0.9609 | -167.1 | 999999 | |
| 1.35 | -5.00 | 2.37 | -5.00 | -17.90 | 145.26 | 73.00 | 251.72 | 0.9597 | -325.7 | 999999 | |
| 1.17 | -5.00 | 2.03 | -5.00 | -18.09 | 145.13 | 72.88 | 251.51 | 0.9592 | -307.0 | 999999 | |
| 1.62 | 55.66 | 2.90 | 95.28 | -20.01 | 145.54 | 73.29 | 249.54 | 0.9617 | -333.4 | -64.2 | |
| 8.39 | -9.00 | 14.16 | -9.00 | -19.29 | 144.59 | 72.33 | 250.22 | 0.9570 | 413.3 | 999999 | |
| 3.79 | -9.00 | 6.53 | -9.00 | -20.18 | 144.97 | 72.71 | 249.32 | 0.9592 | -594.0 | 999999 | |
| 3.07 | 16.24 | 5.34 | 28.29 | -21.09 | 145.08 | 72.82 | 248.38 | 0.9601 | -176.6 | 176.8 | |
| 4.87 | -12.00 | 8.47 | -12.00 | -21.42 | 145.04 | 72.79 | 248.04 | 0.9601 | 512.7 | 999999 | |
| 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. | |