SDO HMI 2014-05-19 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.57 | 39.41 | 5.29 | 31.66 | -18.06 | 217.56 | 50.51 | 248.66 | 0.7897 | -43.7 | -49.2 | |
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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 |
| 3.42 | 18.08 | 2.81 | 14.84 | -18.41 | 218.54 | 51.48 | 248.47 | 0.8003 | 630.6 | 123.1 | |
| 0.63 | 1.53 | 0.51 | 1.25 | -17.97 | 218.35 | 51.30 | 248.97 | 0.7976 | 761.4 | 627.1 | |
| 0.00 | 1.98 | 0.00 | 1.62 | -18.16 | 218.38 | 51.33 | 248.74 | 0.7982 | 443.0 | 453.2 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -17.79 | 218.18 | 51.12 | 249.15 | 0.7954 | 579.0 | 495.4 | |
| 0.00 | 1.71 | 0.00 | 1.38 | -18.86 | 217.44 | 50.39 | 247.65 | 0.7905 | -587.0 | -457.5 | |
| 0.00 | 1.98 | 0.00 | 1.53 | -15.83 | 216.08 | 49.03 | 251.13 | 0.7699 | -722.0 | -536.7 | |
| 0.00 | 2.79 | 0.00 | 2.22 | -18.64 | 217.01 | 49.95 | 247.80 | 0.7857 | -524.0 | -588.7 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -16.58 | 216.14 | 49.08 | 250.18 | 0.7721 | -556.0 | -407.2 | |
| 1.62 | 3.42 | 1.28 | 2.70 | -18.40 | 216.66 | 49.61 | 248.01 | 0.7816 | -555.3 | -436.8 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -18.38 | 216.35 | 49.30 | 247.96 | 0.7784 | -346.0 | -276.3 | |
| 0.90 | 3.87 | 0.69 | 2.97 | -17.13 | 215.51 | 48.45 | 249.32 | 0.7668 | -295.0 | -59.5 | |
| 0.00 | 1.17 | 0.00 | 0.90 | -17.45 | 215.28 | 48.23 | 248.85 | 0.7652 | -697.0 | -643.2 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -17.40 | 213.94 | 46.89 | 248.55 | 0.7507 | 539.0 | 456.0 | |
| 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. | |