SDO HMI 2014-05-18 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.33 | 40.27 | 9.13 | 29.95 | -17.88 | 217.45 | 46.54 | 247.86 | 0.7480 | -203.3 | -145.1 | |
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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 |
| 3.87 | 17.44 | 2.92 | 13.17 | -18.27 | 218.18 | 47.27 | 247.57 | 0.7569 | 402.1 | -38.1 | |
| 1.89 | 4.67 | 1.41 | 3.50 | -17.61 | 217.95 | 47.04 | 248.35 | 0.7527 | 719.2 | 545.6 | |
| 0.81 | -1.00 | 0.61 | -1.00 | -18.56 | 218.24 | 47.33 | 247.22 | 0.7582 | -442.0 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -16.66 | 216.95 | 46.04 | 249.31 | 0.7394 | 354.0 | 303.1 | |
| 0.00 | 2.07 | 0.00 | 1.54 | -18.87 | 217.36 | 46.45 | 246.55 | 0.7499 | -622.0 | -513.1 | |
| 1.35 | 4.76 | 1.00 | 3.52 | -18.34 | 216.99 | 46.08 | 247.13 | 0.7444 | -600.9 | -537.2 | |
| 0.99 | 7.55 | 0.71 | 5.46 | -16.31 | 216.21 | 45.29 | 249.58 | 0.7302 | -545.6 | -369.2 | |
| 0.54 | -6.00 | 0.40 | -6.00 | -18.53 | 216.92 | 46.01 | 246.85 | 0.7441 | -709.2 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.93 | -18.84 | 217.03 | 46.12 | 246.48 | 0.7462 | -762.0 | -621.2 | |
| 2.88 | -7.00 | 2.08 | -7.00 | -16.56 | 216.19 | 45.28 | 249.24 | 0.7307 | -577.2 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.97 | -17.33 | 215.53 | 44.61 | 248.00 | 0.7254 | -579.0 | -574.4 | |
| 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. | |