SDO HMI 2014-08-11 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.49 | 64.82 | 13.34 | 40.22 | -17.86 | 161.62 | 28.25 | 228.46 | 0.6045 | 697.5 | 451.3 | |
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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 | 1.35 | 0.00 | 0.88 | -17.24 | 166.24 | 32.87 | 233.43 | 0.6476 | 236.0 | 278.3 | |
| 19.32 | 42.53 | 12.00 | 26.36 | -17.13 | 162.32 | 28.95 | 230.12 | 0.6050 | 933.8 | 525.7 | |
| 2.17 | -2.00 | 1.34 | -2.00 | -16.97 | 161.89 | 28.52 | 229.92 | 0.5991 | 1019.8 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.96 | -18.62 | 161.71 | 28.34 | 227.59 | 0.6114 | 710.0 | 579.0 | |
| 0.00 | 5.96 | 0.00 | 3.70 | -18.62 | 161.09 | 27.72 | 226.97 | 0.6051 | 870.0 | 682.7 | |
| 0.00 | 0.63 | 0.00 | 0.40 | -20.25 | 160.77 | 27.40 | 224.63 | 0.6168 | 568.0 | 473.3 | |
| 0.00 | 1.63 | 0.00 | 1.02 | -20.04 | 160.58 | 27.21 | 224.69 | 0.6130 | 692.0 | 574.4 | |
| 0.00 | 2.89 | 0.00 | 1.80 | -19.79 | 160.28 | 26.91 | 224.69 | 0.6078 | 774.0 | 639.0 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -19.49 | 159.83 | 26.46 | 224.58 | 0.6006 | 828.0 | 677.5 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -19.45 | 159.64 | 26.27 | 224.44 | 0.5984 | 647.0 | 632.0 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -20.55 | 159.37 | 26.00 | 222.80 | 0.6063 | 614.0 | 599.5 | |
| 0.00 | 1.26 | 0.00 | 0.77 | -18.88 | 158.97 | 25.60 | 224.43 | 0.5863 | 686.0 | 537.1 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -18.45 | 158.58 | 25.21 | 224.53 | 0.5784 | 652.0 | 561.1 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -20.01 | 158.20 | 24.83 | 222.16 | 0.5900 | -793.0 | -698.4 | |
| 0.00 | 2.89 | 0.00 | 1.77 | -20.59 | 157.47 | 24.10 | 220.65 | 0.5891 | -683.0 | -667.3 | |
| 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. | |