SDO HMI 2014-07-14 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.38 | 330.85 | 112.67 | 641.65 | -7.79 | 221.99 | 74.42 | 260.80 | 0.9678 | 502.4 | 195.0 | |
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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 | 2.09 | 0.00 | 3.80 | -4.71 | 221.35 | 73.78 | 263.89 | 0.9636 | -3.0 | 19.0 | |
| 55.93 | 305.33 | 110.29 | 599.99 | -7.77 | 222.20 | 74.63 | 260.84 | 0.9688 | 545.3 | 197.7 | |
| 0.00 | 1.09 | 0.00 | 1.83 | -5.99 | 219.82 | 72.25 | 262.40 | 0.9569 | -254.0 | -282.4 | |
| 0.00 | 1.36 | 0.00 | 2.27 | -6.31 | 219.63 | 72.06 | 262.04 | 0.9561 | -358.0 | -304.9 | |
| 0.00 | 1.27 | 0.00 | 2.16 | -7.35 | 219.92 | 72.35 | 260.99 | 0.9581 | 296.0 | 268.6 | |
| 0.00 | 5.54 | 0.00 | 8.98 | -6.77 | 219.09 | 71.52 | 261.50 | 0.9536 | 204.0 | 213.0 | |
| 0.00 | 1.73 | 0.00 | 2.79 | -7.44 | 218.95 | 71.38 | 260.78 | 0.9533 | 357.0 | 362.1 | |
| 0.00 | 0.73 | 0.00 | 1.16 | -6.96 | 218.77 | 71.20 | 261.26 | 0.9520 | 504.0 | 503.2 | |
| 0.00 | 3.18 | 0.00 | 5.23 | -9.56 | 219.01 | 71.44 | 258.59 | 0.9550 | 368.0 | 258.6 | |
| 1.45 | 7.08 | 2.38 | 11.61 | -9.80 | 218.84 | 71.27 | 258.32 | 0.9543 | 173.9 | 222.3 | |
| 0.00 | 0.54 | 0.00 | 0.71 | -12.41 | 213.67 | 66.10 | 254.74 | 0.9271 | 214.0 | 284.2 | |
| 0.00 | 0.91 | 0.00 | 1.12 | -12.27 | 212.09 | 64.52 | 254.60 | 0.9166 | -251.0 | -205.8 | |
| 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. | |