SDO HMI 2014-05-16 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 |
| 25.70 | 131.47 | 18.77 | 95.62 | 15.37 | 249.09 | 44.00 | 293.80 | 0.7343 | -321.8 | -250.0 | |
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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 |
| 0.00 | 0.81 | 0.00 | 0.60 | 13.72 | 250.95 | 45.86 | 290.94 | 0.7487 | 472.0 | 372.1 | |
| 0.00 | 1.26 | 0.00 | 0.93 | 14.18 | 250.66 | 45.57 | 291.64 | 0.7472 | 575.0 | 454.0 | |
| 15.18 | 120.85 | 11.14 | 88.27 | 15.54 | 249.52 | 44.42 | 293.84 | 0.7396 | -698.4 | -319.3 | |
| 8.09 | -3.00 | 5.87 | -3.00 | 15.52 | 248.98 | 43.89 | 294.04 | 0.7337 | -937.6 | 999999 | |
| 2.43 | -3.00 | 1.76 | -3.00 | 15.77 | 248.74 | 43.65 | 294.46 | 0.7321 | -836.6 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.75 | 11.72 | 247.34 | 42.25 | 289.64 | 0.7013 | 584.0 | 475.2 | |
| 0.00 | 1.71 | 0.00 | 1.19 | 13.26 | 247.44 | 42.35 | 291.70 | 0.7080 | 556.0 | 404.4 | |
| 0.00 | 1.35 | 0.00 | 0.93 | 11.71 | 246.79 | 41.70 | 289.83 | 0.6948 | 563.0 | 489.6 | |
| 0.00 | 0.72 | 0.00 | 0.51 | 16.95 | 247.55 | 42.46 | 296.53 | 0.7240 | -415.0 | -363.1 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 11.56 | 245.94 | 40.84 | 289.97 | 0.6840 | 647.0 | 539.2 | |
| 0.00 | 0.63 | 0.00 | 0.43 | 13.54 | 246.08 | 40.99 | 292.66 | 0.6933 | 538.0 | 460.0 | |
| 0.00 | 1.08 | 0.00 | 0.71 | 10.11 | 244.41 | 39.31 | 288.52 | 0.6601 | 583.0 | 480.4 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 14.53 | 242.21 | 37.11 | 295.99 | 0.6521 | 470.0 | 509.2 | |
| 0.00 | 0.72 | 0.00 | 0.46 | 16.49 | 239.03 | 33.94 | 300.76 | 0.6253 | 602.0 | 525.6 | |
| 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. | |