SDO HMI 2014-09-14 03:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.19 | 65.04 | 11.47 | 36.86 | -15.65 | 65.69 | 18.23 | 218.20 | 0.4895 | 659.2 | 454.9 | |
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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 | 0.98 | 0.00 | 0.57 | -16.71 | 67.75 | 20.29 | 219.83 | 0.5207 | 655.0 | 540.4 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -16.51 | 66.93 | 19.47 | 218.93 | 0.5106 | 689.0 | 577.1 | |
| 0.89 | 1.96 | 0.51 | 1.12 | -15.81 | 66.79 | 19.33 | 219.63 | 0.5013 | 816.1 | 675.2 | |
| 0.89 | 1.96 | 0.51 | 1.12 | -15.86 | 66.40 | 18.94 | 218.99 | 0.4981 | 749.9 | 603.7 | |
| 6.67 | 53.91 | 3.79 | 30.54 | -15.58 | 66.11 | 18.64 | 218.92 | 0.4922 | 898.1 | 532.5 | |
| 3.47 | -5.00 | 1.97 | -5.00 | -15.39 | 66.05 | 18.59 | 219.11 | 0.4894 | 1073.8 | 999999 | |
| 8.27 | -5.00 | 4.69 | -5.00 | -15.34 | 65.82 | 18.36 | 218.81 | 0.4866 | 1113.7 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -14.22 | 63.02 | 15.56 | 215.75 | 0.4470 | 763.0 | 577.4 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -17.47 | 62.06 | 14.60 | 210.16 | 0.4807 | -609.0 | -470.2 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -16.89 | 61.69 | 14.23 | 210.15 | 0.4702 | -705.0 | -597.0 | |
| 0.00 | 1.69 | 0.00 | 0.95 | -16.92 | 61.43 | 13.97 | 209.67 | 0.4686 | -818.0 | -578.2 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -21.92 | 59.47 | 12.01 | 201.73 | 0.5236 | 659.0 | 553.1 | |
| 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. | |