SDO HMI 2014-03-08 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.07 | 160.68 | 25.18 | 91.71 | 14.00 | 50.78 | 20.86 | 315.97 | 0.4986 | -162.2 | -143.2 | |
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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 | 2.25 | 0.00 | 1.30 | 11.88 | 54.69 | 24.77 | 307.64 | 0.5198 | -785.0 | -637.4 | |
| 0.00 | 1.13 | 0.00 | 0.66 | 14.36 | 54.96 | 25.04 | 311.02 | 0.5457 | -660.0 | -520.8 | |
| 0.00 | 1.90 | 0.00 | 1.11 | 13.24 | 54.77 | 24.84 | 309.62 | 0.5330 | -646.0 | -496.1 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 13.46 | 54.76 | 24.83 | 309.95 | 0.5350 | -719.0 | -557.0 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 14.23 | 54.81 | 24.89 | 311.00 | 0.5427 | -633.0 | -451.9 | |
| 0.00 | 1.21 | 0.00 | 0.71 | 14.45 | 54.77 | 24.85 | 311.36 | 0.5443 | -554.0 | -468.1 | |
| 6.92 | 10.13 | 4.06 | 5.94 | 13.84 | 54.66 | 24.74 | 310.61 | 0.5374 | -889.8 | -622.0 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 12.33 | 54.43 | 24.51 | 308.64 | 0.5210 | -808.0 | -584.0 | |
| 0.00 | 1.90 | 0.00 | 1.11 | 13.63 | 54.44 | 24.52 | 310.57 | 0.5330 | -668.0 | -559.4 | |
| 0.00 | 1.13 | 0.00 | 0.66 | 13.78 | 54.22 | 24.30 | 311.04 | 0.5320 | -688.0 | -533.1 | |
| 7.27 | 14.11 | 4.22 | 8.20 | 13.07 | 54.04 | 24.12 | 310.21 | 0.5233 | -998.0 | -682.7 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 13.41 | 53.78 | 23.85 | 311.02 | 0.5235 | -730.0 | -634.4 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 11.09 | 53.45 | 23.53 | 307.84 | 0.4981 | -761.0 | -678.5 | |
| 0.87 | 3.03 | 0.50 | 1.75 | 13.19 | 53.35 | 23.43 | 311.21 | 0.5167 | -991.6 | -804.7 | |
| 0.00 | 1.47 | 0.00 | 0.85 | 13.48 | 53.32 | 23.39 | 311.68 | 0.5190 | -745.0 | -525.4 | |
| 2.08 | 3.98 | 1.20 | 2.30 | 13.69 | 53.07 | 23.15 | 312.29 | 0.5184 | -855.8 | -644.2 | |
| 0.00 | 1.04 | 0.00 | 0.60 | 13.46 | 52.98 | 23.06 | 312.07 | 0.5152 | -727.0 | -612.0 | |
| 0.00 | 2.60 | 0.00 | 1.47 | 11.38 | 52.45 | 22.53 | 309.53 | 0.4890 | -932.0 | -816.7 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 13.56 | 52.53 | 22.60 | 312.79 | 0.5112 | -751.0 | -590.6 | |
| 0.00 | 1.82 | 0.00 | 1.03 | 11.15 | 52.17 | 22.25 | 309.51 | 0.4835 | -726.0 | -546.0 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 16.16 | 52.45 | 22.53 | 316.51 | 0.5368 | -550.0 | -427.8 | |
| 2.51 | 12.03 | 1.45 | 6.95 | 14.41 | 52.15 | 22.23 | 314.49 | 0.5156 | -974.4 | -734.0 | |
| 0.00 | 2.42 | 0.00 | 1.41 | 15.50 | 52.24 | 22.32 | 315.90 | 0.5279 | -825.0 | -641.5 | |
| 0.00 | 1.13 | 0.00 | 0.64 | 13.09 | 51.98 | 22.06 | 312.78 | 0.5005 | -712.0 | -584.8 | |
| 2.51 | -22.00 | 1.45 | -22.00 | 14.72 | 52.08 | 22.16 | 315.02 | 0.5182 | -968.2 | 999999 | |
| 2.25 | 9.43 | 1.28 | 5.38 | 13.30 | 51.71 | 21.78 | 313.46 | 0.4996 | -1021.7 | -764.0 | |
| 0.00 | 1.30 | 0.00 | 0.75 | 14.26 | 51.80 | 21.88 | 314.73 | 0.5105 | -664.0 | -561.6 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 14.90 | 51.81 | 21.88 | 315.63 | 0.5171 | -674.0 | -556.2 | |
| 0.00 | 1.38 | 0.00 | 0.81 | 16.52 | 51.99 | 22.07 | 317.58 | 0.5361 | -589.0 | -481.6 | |
| 0.00 | 3.98 | 0.00 | 2.28 | 13.87 | 51.53 | 21.61 | 314.52 | 0.5035 | -866.0 | -745.4 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 15.64 | 51.69 | 21.76 | 316.79 | 0.5236 | -726.0 | -651.6 | |
| 0.00 | 1.47 | 0.00 | 0.82 | 9.47 | 50.81 | 20.89 | 308.46 | 0.4510 | -709.0 | -514.8 | |
| 0.00 | 1.13 | 0.00 | 0.65 | 14.95 | 50.82 | 20.90 | 317.02 | 0.5075 | 466.0 | 418.0 | |
| 2.68 | 6.66 | 1.53 | 3.79 | 13.85 | 50.54 | 20.62 | 315.84 | 0.4928 | 797.8 | 502.2 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 14.07 | 50.40 | 20.48 | 316.35 | 0.4937 | 535.0 | 547.3 | |
| 0.00 | 1.64 | 0.00 | 0.93 | 13.29 | 50.00 | 20.08 | 315.77 | 0.4810 | 847.0 | 730.5 | |
| 0.00 | 2.08 | 0.00 | 1.19 | 15.79 | 49.42 | 19.50 | 320.11 | 0.5029 | 797.0 | 705.4 | |
| 1.99 | 6.49 | 1.12 | 3.66 | 14.24 | 49.11 | 19.19 | 318.44 | 0.4822 | -705.9 | -485.8 | |
| 0.00 | 1.82 | 0.00 | 1.02 | 13.77 | 48.58 | 18.66 | 318.57 | 0.4716 | 779.0 | 600.1 | |
| 0.00 | 1.82 | 0.00 | 1.00 | 11.73 | 48.20 | 18.28 | 316.08 | 0.4446 | 737.0 | 512.1 | |
| 0.00 | 1.30 | 0.00 | 0.73 | 13.88 | 48.14 | 18.22 | 319.41 | 0.4684 | 539.0 | 492.5 | |
| 0.00 | 1.82 | 0.00 | 1.03 | 16.22 | 48.09 | 18.17 | 322.64 | 0.4954 | 813.0 | 639.9 | |
| 0.00 | 2.60 | 0.00 | 1.47 | 15.27 | 47.81 | 17.89 | 321.84 | 0.4815 | 788.0 | 546.1 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 14.27 | 47.62 | 17.70 | 320.77 | 0.4679 | 743.0 | 536.4 | |
| 7.10 | 11.34 | 3.98 | 6.36 | 14.80 | 47.28 | 17.36 | 322.04 | 0.4710 | 884.6 | 635.4 | |
| 0.00 | 3.46 | 0.00 | 1.93 | 14.19 | 47.23 | 17.31 | 321.29 | 0.4632 | 918.0 | 759.3 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 12.91 | 47.07 | 17.15 | 319.72 | 0.4464 | 358.0 | 328.1 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 14.92 | 46.97 | 17.05 | 322.70 | 0.4694 | 741.0 | 667.6 | |
| 0.00 | 0.87 | 0.00 | 0.48 | 13.91 | 46.66 | 16.74 | 321.83 | 0.4544 | 768.0 | 491.8 | |
| 0.35 | 2.86 | 0.19 | 1.60 | 15.09 | 46.44 | 16.51 | 323.80 | 0.4666 | 809.5 | 602.1 | |
| 2.34 | 17.57 | 1.30 | 9.80 | 14.73 | 46.22 | 16.29 | 323.69 | 0.4602 | 1102.7 | 751.8 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 15.76 | 46.24 | 16.31 | 324.99 | 0.4731 | 564.0 | 448.8 | |
| 2.60 | -51.00 | 1.45 | -51.00 | 15.18 | 46.12 | 16.20 | 324.43 | 0.4649 | 924.6 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 15.56 | 46.15 | 16.23 | 324.88 | 0.4700 | 724.0 | 591.0 | |
| 2.60 | -51.00 | 1.45 | -51.00 | 14.92 | 46.04 | 16.12 | 324.24 | 0.4609 | 1026.5 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.58 | 15.92 | 45.28 | 15.36 | 326.78 | 0.4670 | 796.0 | 624.4 | |
| 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. | |