SDO HMI 2014-07-07 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.73 | 13.82 | 0.47 | 9.35 | -22.27 | 199.89 | -34.84 | 129.11 | 0.6807 | 63.4 | -17.6 | |
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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 | 0.82 | 0.00 | 0.52 | -21.44 | 205.23 | -29.50 | 132.16 | 0.6205 | 640.0 | 449.7 | |
| 0.73 | 2.36 | 0.47 | 1.51 | -22.87 | 204.82 | -29.91 | 133.59 | 0.6366 | -773.6 | -658.9 | |
| 0.00 | 0.73 | 0.00 | 0.46 | -21.81 | 204.31 | -30.41 | 131.80 | 0.6328 | 581.0 | 471.2 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -21.01 | 204.16 | -30.57 | 130.64 | 0.6279 | 674.0 | 580.5 | |
| 0.00 | 0.82 | 0.00 | 0.56 | -26.30 | 202.25 | -32.48 | 135.45 | 0.6885 | -293.0 | -268.3 | |
| 0.00 | 1.09 | 0.00 | 0.71 | -22.57 | 202.81 | -31.91 | 131.47 | 0.6538 | 536.0 | 440.7 | |
| 0.00 | 0.64 | 0.00 | 0.41 | -20.88 | 202.08 | -32.65 | 128.73 | 0.6485 | 392.0 | 474.4 | |
| 0.00 | 1.09 | 0.00 | 0.71 | -20.62 | 201.87 | -32.86 | 128.23 | 0.6487 | 651.0 | 532.9 | |
| 0.00 | 1.09 | 0.00 | 0.77 | -24.48 | 198.00 | -36.73 | 130.12 | 0.7141 | 449.0 | 368.9 | |
| 0.00 | 1.00 | 0.00 | 0.71 | -21.64 | 195.92 | -38.81 | 125.33 | 0.7163 | -190.0 | -266.0 | |
| 0.00 | 1.27 | 0.00 | 0.91 | -21.17 | 195.05 | -39.67 | 124.22 | 0.7222 | -448.0 | -406.6 | |
| 0.00 | 0.91 | 0.00 | 0.68 | -21.83 | 192.12 | -42.61 | 123.34 | 0.7545 | -511.0 | -508.0 | |
| 0.00 | 1.09 | 0.00 | 0.82 | -21.97 | 191.97 | -42.75 | 123.43 | 0.7566 | -490.0 | -447.8 | |
| 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. | |