SDO HMI 2014-04-16 11:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.86 | 82.41 | 11.18 | 78.21 | -13.27 | 181.06 | -58.87 | 102.21 | 0.8545 | 65.7 | -41.1 | |
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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 | 1.06 | 0.00 | 1.02 | -15.96 | 180.83 | -59.10 | 105.34 | 0.8575 | -259.0 | -253.6 | |
| 0.00 | 1.33 | 0.00 | 1.23 | -12.75 | 182.01 | -57.92 | 101.63 | 0.8458 | -513.0 | -487.4 | |
| 10.53 | 60.01 | 9.91 | 56.61 | -13.65 | 181.31 | -58.62 | 102.66 | 0.8524 | 621.0 | 80.5 | |
| 0.00 | 0.89 | 0.00 | 0.83 | -11.52 | 181.20 | -58.73 | 100.16 | 0.8529 | -542.0 | -470.3 | |
| 0.00 | 0.62 | 0.00 | 0.59 | -11.63 | 181.04 | -58.88 | 100.29 | 0.8543 | -359.0 | -334.4 | |
| 1.33 | 4.51 | 1.27 | 4.32 | -11.60 | 180.63 | -59.29 | 100.24 | 0.8579 | 351.5 | 200.5 | |
| 0.00 | 2.21 | 0.00 | 2.13 | -12.10 | 180.45 | -59.48 | 100.83 | 0.8596 | -629.0 | -552.5 | |
| 0.00 | 2.57 | 0.00 | 2.49 | -12.42 | 180.21 | -59.72 | 101.20 | 0.8617 | -664.0 | -547.5 | |
| 0.00 | 2.57 | 0.00 | 2.48 | -11.91 | 180.28 | -59.65 | 100.60 | 0.8611 | -332.0 | -378.9 | |
| 0.00 | 1.06 | 0.00 | 1.03 | -12.11 | 180.14 | -59.78 | 100.83 | 0.8623 | -542.0 | -497.5 | |
| 0.00 | 0.80 | 0.00 | 0.79 | -13.05 | 179.59 | -60.34 | 101.91 | 0.8672 | -495.0 | -365.8 | |
| 0.00 | 2.92 | 0.00 | 2.87 | -12.33 | 179.81 | -60.12 | 101.08 | 0.8651 | -460.0 | -323.3 | |
| 0.00 | 1.86 | 0.00 | 1.82 | -12.08 | 179.78 | -60.15 | 100.79 | 0.8654 | -348.0 | -258.9 | |
| 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. | |