SDO HMI 2014-02-26 21:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.79 | 34.20 | 14.61 | 35.91 | 15.81 | 102.59 | -57.96 | 67.71 | 0.8825 | -145.8 | -28.4 | |
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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 | 1.38 | 0.00 | 1.15 | 10.09 | 109.70 | -50.86 | 71.76 | 0.8062 | 665.0 | 548.9 | |
| 0.00 | 0.43 | 0.00 | 0.37 | 10.99 | 108.76 | -51.80 | 71.03 | 0.8179 | 354.0 | 357.0 | |
| 0.00 | 1.12 | 0.00 | 1.12 | 16.12 | 104.21 | -56.34 | 66.84 | 0.8718 | -684.0 | -560.5 | |
| 0.00 | 1.38 | 0.00 | 1.40 | 16.67 | 103.85 | -56.70 | 66.37 | 0.8760 | -436.0 | -330.1 | |
| 0.00 | 0.69 | 0.00 | 0.71 | 17.20 | 103.43 | -57.12 | 65.94 | 0.8806 | -247.0 | -249.2 | |
| 3.88 | 15.33 | 3.93 | 15.52 | 16.19 | 103.84 | -56.71 | 66.89 | 0.8748 | -395.3 | -46.6 | |
| 4.48 | -6.00 | 4.51 | -6.00 | 15.83 | 103.94 | -56.61 | 67.25 | 0.8731 | -368.7 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.70 | 15.26 | 103.62 | -56.94 | 67.98 | 0.8741 | 407.0 | 360.5 | |
| 0.00 | 0.60 | 0.00 | 0.63 | 15.70 | 102.79 | -57.76 | 67.77 | 0.8816 | -217.0 | -212.7 | |
| 2.50 | 8.53 | 2.76 | 9.46 | 16.10 | 100.99 | -59.56 | 67.92 | 0.8958 | -456.3 | -329.5 | |
| 2.24 | -10.00 | 2.49 | -10.00 | 15.97 | 100.68 | -59.87 | 68.15 | 0.8977 | -279.6 | 999999 | |
| 0.00 | 0.52 | 0.00 | 0.56 | 14.75 | 101.14 | -59.42 | 69.33 | 0.8917 | 494.0 | 495.5 | |
| 0.00 | 0.86 | 0.00 | 0.95 | 15.16 | 100.89 | -59.66 | 68.96 | 0.8944 | 518.0 | 476.3 | |
| 0.00 | 0.95 | 0.00 | 1.05 | 15.02 | 100.71 | -59.85 | 69.17 | 0.8954 | 410.0 | 363.5 | |
| 0.69 | 1.72 | 0.92 | 2.29 | 17.23 | 96.16 | -64.40 | 68.15 | 0.9297 | 346.6 | 286.4 | |
| 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. | |