SDO HMI 2014-05-19 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.66 | 40.85 | 5.61 | 34.12 | -18.21 | 217.71 | 52.30 | 248.89 | 0.8077 | 40.0 | 60.0 | |
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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 |
| 4.32 | 21.14 | 3.69 | 18.03 | -18.44 | 218.64 | 53.23 | 248.82 | 0.8171 | 740.5 | 280.4 | |
| 0.36 | 1.35 | 0.31 | 1.15 | -18.06 | 218.47 | 53.06 | 249.24 | 0.8148 | 639.5 | 577.0 | |
| 0.00 | 1.80 | 0.00 | 1.52 | -17.91 | 218.30 | 52.89 | 249.38 | 0.8129 | 514.0 | 432.5 | |
| 0.00 | 0.99 | 0.00 | 0.82 | -16.95 | 217.54 | 52.13 | 250.39 | 0.8038 | 500.0 | 450.7 | |
| 0.00 | 1.98 | 0.00 | 1.66 | -18.82 | 217.58 | 52.17 | 248.12 | 0.8079 | -510.0 | -464.1 | |
| 0.54 | 2.52 | 0.45 | 2.08 | -18.64 | 217.14 | 51.73 | 248.23 | 0.8032 | -588.5 | -453.8 | |
| 0.00 | 1.35 | 0.00 | 1.08 | -15.74 | 215.92 | 50.51 | 251.56 | 0.7853 | -616.0 | -499.9 | |
| 0.81 | 3.87 | 0.66 | 3.15 | -18.47 | 216.50 | 51.09 | 248.29 | 0.7966 | -560.8 | -279.3 | |
| 0.00 | 0.72 | 0.00 | 0.58 | -18.41 | 216.22 | 50.81 | 248.29 | 0.7938 | -490.0 | -400.5 | |
| 0.00 | 0.90 | 0.00 | 0.72 | -18.20 | 215.93 | 50.52 | 248.48 | 0.7904 | -174.0 | -258.4 | |
| 0.63 | 1.98 | 0.50 | 1.57 | -17.20 | 215.30 | 49.89 | 249.57 | 0.7819 | -401.1 | -436.3 | |
| 0.00 | 1.26 | 0.00 | 1.00 | -17.52 | 215.37 | 49.96 | 249.19 | 0.7832 | -543.0 | -395.6 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -17.52 | 214.00 | 48.59 | 248.84 | 0.7691 | 238.0 | 263.9 | |
| 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. | |