SDO HMI 2014-02-25 01:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.67 | 240.52 | 77.23 | 508.41 | -13.10 | 107.29 | -77.41 | 101.80 | 0.9715 | -274.8 | -315.2 | |
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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 | 2.07 | 0.00 | 1.76 | -11.90 | 129.53 | -55.16 | 99.53 | 0.8166 | 489.0 | 409.4 | |
| 0.00 | 0.77 | 0.00 | 0.71 | -11.32 | 126.84 | -57.86 | 98.88 | 0.8425 | 534.0 | 482.3 | |
| 0.00 | 0.77 | 0.00 | 0.72 | -11.06 | 126.17 | -58.53 | 98.60 | 0.8487 | 191.0 | 253.1 | |
| 0.00 | 1.29 | 0.00 | 1.18 | -5.72 | 127.00 | -57.70 | 92.22 | 0.8438 | 157.0 | 224.3 | |
| 0.00 | 0.86 | 0.00 | 0.84 | -2.81 | 124.93 | -59.76 | 89.07 | 0.8651 | 333.0 | 282.5 | |
| 0.00 | 1.29 | 0.00 | 1.89 | -16.05 | 113.33 | -71.37 | 104.54 | 0.9422 | 417.0 | 275.8 | |
| 0.00 | 0.60 | 0.00 | 0.99 | -12.56 | 111.24 | -73.45 | 100.95 | 0.9544 | -454.0 | -504.6 | |
| 0.00 | 1.64 | 0.00 | 2.74 | -11.82 | 110.92 | -73.78 | 100.20 | 0.9562 | 159.0 | 37.9 | |
| 10.24 | 222.10 | 21.15 | 475.88 | -14.16 | 107.27 | -77.43 | 102.88 | 0.9719 | -617.0 | -340.7 | |
| 0.00 | 4.48 | 0.00 | 10.53 | -15.20 | 105.44 | -79.25 | 104.08 | 0.9784 | 220.0 | 219.1 | |
| 0.00 | 3.27 | 0.00 | 7.80 | -14.75 | 105.25 | -79.44 | 103.63 | 0.9792 | -420.0 | -381.4 | |
| 26.43 | -9.00 | 56.08 | -9.00 | -12.66 | 107.04 | -77.65 | 101.36 | 0.9732 | -221.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 3.37 | -13.55 | 105.03 | -79.67 | 102.43 | 0.9803 | -428.0 | -382.2 | |
| 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. | |