SDO HMI 2014-05-16 20:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.42 | 42.67 | 5.32 | 21.77 | -15.49 | 193.74 | -4.73 | 160.47 | 0.2403 | 323.5 | 414.4 | |
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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 | 0.99 | 0.00 | 0.50 | -16.12 | 195.11 | -3.37 | 166.54 | 0.2434 | 941.0 | 737.3 | |
| 3.95 | 7.36 | 2.02 | 3.77 | -16.50 | 195.07 | -3.40 | 166.76 | 0.2497 | 1170.8 | 780.8 | |
| 1.08 | 2.96 | 0.55 | 1.51 | -15.62 | 194.71 | -3.77 | 164.44 | 0.2369 | 913.1 | 673.4 | |
| 0.00 | 2.60 | 0.00 | 1.33 | -16.49 | 194.50 | -3.97 | 164.64 | 0.2521 | 904.0 | 697.9 | |
| 0.00 | 1.98 | 0.00 | 1.00 | -12.56 | 194.52 | -3.96 | 158.91 | 0.1882 | -1013.0 | -810.5 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -15.22 | 194.25 | -4.23 | 162.09 | 0.2326 | 572.0 | 436.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.06 | 193.87 | -4.61 | 160.39 | 0.2321 | 994.0 | 870.2 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -15.52 | 193.74 | -4.74 | 160.55 | 0.2403 | -833.0 | -540.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.03 | 193.65 | -4.83 | 159.49 | 0.2329 | 1033.0 | 888.5 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -15.80 | 193.29 | -5.19 | 159.29 | 0.2474 | -106.0 | -162.8 | |
| 1.26 | 11.32 | 0.64 | 5.77 | -15.27 | 193.27 | -5.21 | 158.41 | 0.2391 | 1036.2 | 812.9 | |
| 0.00 | 2.16 | 0.00 | 1.10 | -14.90 | 192.81 | -5.67 | 156.05 | 0.2363 | 840.0 | 637.2 | |
| 4.13 | 7.54 | 2.11 | 3.86 | -15.36 | 192.41 | -6.06 | 155.44 | 0.2462 | -1056.4 | -746.9 | |
| 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. | |