SDO HMI 2014-05-19 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.82 | 179.00 | 30.44 | 107.25 | -16.92 | 195.11 | 31.34 | 242.44 | 0.5632 | 61.4 | -6.4 | |
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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 | 0.72 | 0.00 | 0.45 | -19.24 | 198.01 | 34.25 | 240.57 | 0.6123 | 538.0 | 500.6 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -18.36 | 197.31 | 33.54 | 241.49 | 0.5990 | -136.0 | -84.8 | |
| 0.54 | 88.69 | 0.33 | 54.30 | -18.24 | 197.02 | 33.25 | 241.50 | 0.5947 | 626.7 | 360.9 | |
| 16.73 | -3.00 | 10.24 | -3.00 | -17.83 | 196.82 | 33.05 | 242.02 | 0.5901 | 998.5 | 999999 | |
| 6.48 | -3.00 | 3.96 | -3.00 | -18.09 | 196.64 | 32.87 | 241.51 | 0.5893 | 983.8 | 999999 | |
| 2.97 | -3.00 | 1.80 | -3.00 | -17.31 | 196.37 | 32.60 | 242.58 | 0.5816 | 973.1 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -16.83 | 194.85 | 31.09 | 242.41 | 0.5598 | 861.0 | 624.5 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -17.47 | 194.30 | 30.54 | 240.98 | 0.5564 | 747.0 | 614.2 | |
| 0.00 | 0.45 | 0.00 | 0.27 | -16.60 | 193.78 | 30.01 | 242.08 | 0.5446 | -528.0 | -413.8 | |
| 0.27 | 83.65 | 0.16 | 48.97 | -15.88 | 193.55 | 29.79 | 243.15 | 0.5376 | -782.3 | -433.1 | |
| 11.69 | -10.00 | 6.84 | -10.00 | -15.57 | 193.32 | 29.55 | 243.53 | 0.5328 | -1083.8 | 999999 | |
| 11.06 | -10.00 | 6.48 | -10.00 | -16.14 | 193.34 | 29.57 | 242.57 | 0.5362 | -1027.6 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -14.86 | 192.96 | 29.19 | 244.55 | 0.5242 | 530.0 | 340.7 | |
| 1.08 | -10.00 | 0.63 | -10.00 | -16.27 | 193.07 | 29.30 | 242.16 | 0.5334 | -938.9 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -15.91 | 191.54 | 27.77 | 241.65 | 0.5112 | -725.0 | -557.8 | |
| 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. | |