SDO HMI 2014-05-16 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 |
| 15.54 | 46.73 | 7.93 | 23.80 | -15.66 | 194.12 | -3.25 | 166.45 | 0.2361 | 458.2 | 518.7 | |
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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 | 1.08 | 0.00 | 0.55 | -16.28 | 195.23 | -2.14 | 171.46 | 0.2421 | 1033.0 | 851.8 | |
| 4.31 | 10.87 | 2.20 | 5.56 | -16.62 | 195.16 | -2.21 | 171.41 | 0.2481 | 1086.7 | 861.6 | |
| 2.78 | 6.02 | 1.42 | 3.07 | -15.78 | 195.02 | -2.35 | 170.25 | 0.2343 | 1036.8 | 694.0 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -16.59 | 194.69 | -2.68 | 169.58 | 0.2489 | 950.0 | 772.0 | |
| 0.00 | 1.44 | 0.00 | 0.72 | -12.53 | 194.52 | -2.84 | 164.48 | 0.1818 | -916.0 | -785.3 | |
| 0.45 | 1.62 | 0.23 | 0.82 | -15.31 | 194.27 | -3.10 | 166.77 | 0.2291 | 765.6 | 584.5 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -15.12 | 194.18 | -3.19 | 166.19 | 0.2263 | 812.0 | 676.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.09 | 193.77 | -3.60 | 164.47 | 0.2276 | 879.0 | 743.2 | |
| 0.90 | 14.73 | 0.46 | 7.50 | -15.46 | 193.70 | -3.67 | 164.64 | 0.2340 | -583.4 | 574.1 | |
| 1.71 | -9.00 | 0.87 | -9.00 | -15.40 | 193.60 | -3.76 | 164.19 | 0.2334 | 512.4 | 999999 | |
| 1.98 | -9.00 | 1.01 | -9.00 | -15.24 | 193.42 | -3.95 | 163.25 | 0.2317 | 1059.4 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -14.93 | 192.86 | -4.51 | 160.59 | 0.2296 | 865.0 | 682.5 | |
| 3.41 | 5.75 | 1.74 | 2.93 | -15.33 | 192.41 | -4.96 | 159.45 | 0.2387 | -1030.4 | -778.8 | |
| 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. | |