SDO HMI 2014-05-19 01:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.14 | 48.11 | 10.04 | 36.93 | -17.97 | 217.48 | 48.22 | 248.21 | 0.7661 | -144.7 | -106.0 | |
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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 |
| 5.04 | 21.22 | 3.94 | 16.58 | -18.34 | 218.34 | 49.08 | 247.98 | 0.7760 | 460.6 | -1.0 | |
| 0.00 | 1.08 | 0.00 | 0.84 | -17.55 | 218.04 | 48.79 | 248.90 | 0.7711 | 520.0 | 354.2 | |
| 0.90 | 3.60 | 0.70 | 2.79 | -17.77 | 218.08 | 48.82 | 248.62 | 0.7720 | 747.7 | 509.2 | |
| 0.00 | 1.26 | 0.00 | 0.97 | -18.84 | 217.41 | 48.16 | 247.09 | 0.7677 | -482.0 | -430.9 | |
| 0.00 | 1.08 | 0.00 | 0.83 | -18.65 | 217.29 | 48.04 | 247.29 | 0.7660 | -339.0 | -306.6 | |
| 0.00 | 0.63 | 0.00 | 0.48 | -18.81 | 217.16 | 47.91 | 247.05 | 0.7651 | -561.0 | -503.9 | |
| 0.36 | 1.89 | 0.27 | 1.40 | -16.03 | 216.11 | 46.86 | 250.36 | 0.7469 | -477.2 | -456.2 | |
| 1.89 | 8.18 | 1.44 | 6.23 | -18.56 | 216.92 | 47.67 | 247.29 | 0.7619 | -683.8 | -527.7 | |
| 1.08 | -8.00 | 0.82 | -8.00 | -18.41 | 216.82 | 47.56 | 247.46 | 0.7604 | -637.8 | 999999 | |
| 3.33 | 6.02 | 2.47 | 4.48 | -16.66 | 216.08 | 46.83 | 249.52 | 0.7481 | -479.4 | -178.6 | |
| 0.00 | 1.35 | 0.00 | 1.00 | -17.04 | 216.11 | 46.85 | 249.04 | 0.7493 | 201.0 | 134.7 | |
| 0.54 | 1.80 | 0.40 | 1.33 | -17.40 | 215.44 | 46.19 | 248.37 | 0.7430 | -604.0 | -486.3 | |
| 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. | |