SDO HMI 2014-09-26 14:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 17.74 | 0.49 | 10.82 | 6.88 | 207.11 | -35.92 | 87.84 | 0.5849 | 236.8 | 176.7 | |
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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 | 1.94 | 0.00 | 1.14 | 6.84 | 210.25 | -32.78 | 88.10 | 0.5400 | -725.0 | -585.6 | |
| 0.00 | 1.32 | 0.00 | 0.78 | 6.29 | 209.64 | -33.39 | 89.06 | 0.5493 | -696.0 | -582.7 | |
| 0.00 | 1.59 | 0.00 | 0.95 | 6.26 | 208.80 | -34.23 | 89.03 | 0.5614 | -642.0 | -481.2 | |
| 0.00 | 1.32 | 0.00 | 0.80 | 5.07 | 208.11 | -34.92 | 91.05 | 0.5725 | -579.0 | -417.2 | |
| 0.00 | 1.15 | 0.00 | 0.70 | 5.95 | 206.82 | -36.21 | 89.38 | 0.5898 | 675.0 | 544.1 | |
| 0.00 | 1.32 | 0.00 | 0.81 | 5.31 | 206.83 | -36.20 | 90.45 | 0.5903 | 519.0 | 517.3 | |
| 0.00 | 1.24 | 0.00 | 0.76 | 7.87 | 206.35 | -36.68 | 86.09 | 0.5953 | 805.0 | 684.6 | |
| 0.00 | 1.50 | 0.00 | 0.93 | 7.60 | 205.96 | -37.07 | 86.52 | 0.6008 | 830.0 | 708.2 | |
| 0.00 | 1.50 | 0.00 | 0.93 | 8.17 | 205.86 | -37.17 | 85.58 | 0.6020 | 593.0 | 531.8 | |
| 0.00 | 2.30 | 0.00 | 1.42 | 7.68 | 205.80 | -37.23 | 86.39 | 0.6030 | 544.0 | 481.0 | |
| 0.79 | 1.77 | 0.49 | 1.10 | 7.01 | 205.64 | -37.39 | 87.50 | 0.6056 | 652.4 | 556.5 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 8.08 | 204.68 | -38.35 | 85.69 | 0.6183 | 661.0 | 494.1 | |
| 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. | |