SDO HMI 2014-09-14 01:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.44 | 70.80 | 12.09 | 39.89 | -15.71 | 65.78 | 17.22 | 216.53 | 0.4809 | 635.1 | 446.4 | |
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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 | 0.98 | 0.00 | 0.56 | -16.71 | 67.71 | 19.15 | 218.21 | 0.5101 | 699.0 | 553.1 | |
| 0.98 | 3.47 | 0.56 | 1.97 | -15.82 | 66.80 | 18.24 | 217.99 | 0.4911 | 891.7 | 643.4 | |
| 0.00 | 1.51 | 0.00 | 0.87 | -18.10 | 66.76 | 18.20 | 215.14 | 0.5179 | 611.0 | 389.6 | |
| 0.98 | 2.49 | 0.55 | 1.41 | -15.84 | 66.40 | 17.84 | 217.37 | 0.4877 | 748.8 | 589.7 | |
| 6.05 | 57.81 | 3.42 | 32.54 | -15.60 | 66.15 | 17.59 | 217.29 | 0.4825 | 868.6 | 517.3 | |
| 5.78 | -5.00 | 3.26 | -5.00 | -15.46 | 66.04 | 17.48 | 217.29 | 0.4798 | 976.8 | 999999 | |
| 4.09 | -5.00 | 2.30 | -5.00 | -15.26 | 65.83 | 17.27 | 217.22 | 0.4754 | 1164.2 | 999999 | |
| 3.56 | -5.00 | 2.00 | -5.00 | -15.48 | 65.75 | 17.19 | 216.80 | 0.4774 | 984.9 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -18.33 | 63.24 | 14.68 | 209.36 | 0.4925 | 535.0 | 415.8 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -17.05 | 61.93 | 13.37 | 208.45 | 0.4659 | -628.0 | -526.6 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -16.88 | 61.79 | 13.23 | 208.37 | 0.4626 | -907.0 | -735.6 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -18.23 | 59.00 | 10.44 | 201.90 | 0.4631 | -534.0 | -391.1 | |
| 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. | |