SDO HMI 2014-07-29 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.84 | 248.62 | 101.44 | 555.23 | -7.14 | 227.48 | -76.15 | 98.67 | 0.9751 | 150.5 | -24.4 | |
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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 |
| 22.92 | 142.43 | 44.78 | 282.98 | -7.54 | 229.27 | -74.36 | 99.31 | 0.9685 | 473.5 | 162.9 | |
| 0.00 | 0.45 | 0.00 | 1.09 | -9.43 | 226.75 | -76.88 | 100.89 | 0.9793 | -308.0 | -260.0 | |
| 1.63 | 8.25 | 3.89 | 19.92 | -9.14 | 226.82 | -76.81 | 100.60 | 0.9789 | -209.8 | -288.5 | |
| 2.08 | 5.71 | 5.11 | 14.03 | -8.63 | 226.34 | -77.30 | 100.02 | 0.9803 | -416.3 | -281.5 | |
| 0.00 | 1.09 | 0.00 | 2.45 | -7.30 | 227.16 | -76.48 | 98.79 | 0.9768 | -204.0 | -183.9 | |
| 2.63 | -1.00 | 5.89 | -1.00 | -6.83 | 227.28 | -76.36 | 98.32 | 0.9761 | 125.8 | 999999 | |
| 1.36 | 9.06 | 3.20 | 21.13 | -6.40 | 226.54 | -77.10 | 97.79 | 0.9786 | 183.7 | 154.1 | |
| 0.00 | 1.00 | 0.00 | 2.34 | -5.85 | 226.53 | -77.11 | 97.22 | 0.9784 | 269.0 | 284.1 | |
| 4.62 | 18.48 | 10.54 | 43.23 | -4.65 | 226.74 | -76.89 | 96.04 | 0.9771 | -331.3 | -297.6 | |
| 0.00 | 0.72 | 0.00 | 2.23 | -9.16 | 224.02 | -79.61 | 100.26 | 0.9876 | -382.0 | -346.1 | |
| 10.60 | 49.47 | 28.03 | 135.36 | -7.23 | 225.33 | -78.30 | 98.48 | 0.9830 | 53.2 | -255.7 | |
| 0.00 | 11.33 | 0.00 | 28.93 | -5.79 | 225.53 | -78.10 | 97.04 | 0.9818 | -366.0 | -204.9 | |
| 0.00 | 0.63 | 0.00 | 1.54 | -4.02 | 225.97 | -77.66 | 95.30 | 0.9796 | -428.0 | -398.9 | |
| 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. | |