SDO HMI 2014-07-29 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.85 | 254.60 | 100.01 | 542.90 | -7.23 | 227.56 | -75.52 | 98.84 | 0.9727 | 182.1 | -28.1 | |
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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 |
| 27.27 | 153.47 | 51.44 | 293.72 | -7.55 | 229.30 | -73.78 | 99.40 | 0.9660 | 452.5 | 149.5 | |
| 1.45 | 14.68 | 3.31 | 33.86 | -9.15 | 226.81 | -76.27 | 100.69 | 0.9770 | -242.6 | -219.3 | |
| 0.00 | 2.36 | 0.00 | 5.46 | -9.52 | 226.56 | -76.53 | 101.03 | 0.9781 | -375.0 | -333.5 | |
| 2.54 | -2.00 | 5.91 | -2.00 | -8.62 | 226.50 | -76.58 | 100.11 | 0.9778 | -330.7 | 999999 | |
| 2.54 | -1.00 | 5.46 | -1.00 | -6.84 | 227.25 | -75.83 | 98.40 | 0.9741 | 139.2 | 999999 | |
| 1.18 | 3.90 | 2.66 | 8.87 | -6.38 | 226.56 | -76.52 | 97.84 | 0.9765 | 207.9 | 66.4 | |
| 0.00 | 1.09 | 0.00 | 2.44 | -5.86 | 226.53 | -76.55 | 97.30 | 0.9764 | 262.0 | 289.6 | |
| 2.90 | 21.02 | 6.34 | 47.04 | -4.63 | 226.75 | -76.33 | 96.08 | 0.9750 | -376.1 | -281.3 | |
| 0.82 | -8.00 | 1.81 | -8.00 | -4.87 | 226.53 | -76.55 | 96.30 | 0.9759 | -85.8 | 999999 | |
| 9.15 | 48.38 | 23.08 | 125.97 | -7.25 | 225.24 | -77.84 | 98.55 | 0.9815 | 34.8 | -228.9 | |
| 0.00 | 1.54 | 0.00 | 4.52 | -9.12 | 223.86 | -79.22 | 100.27 | 0.9865 | -389.0 | -359.8 | |
| 0.00 | 6.89 | 0.00 | 16.99 | -5.79 | 225.30 | -77.79 | 97.08 | 0.9807 | -382.0 | -311.2 | |
| 0.00 | 1.27 | 0.00 | 4.03 | -8.86 | 223.04 | -80.04 | 99.90 | 0.9886 | -87.0 | -89.3 | |
| 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. | |