SDO HMI 2014-05-18 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.63 | 254.60 | 39.77 | 137.45 | -16.54 | 194.64 | 18.74 | 231.08 | 0.3972 | 170.8 | -15.2 | |
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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 | 0.72 | 0.00 | 0.40 | -17.77 | 197.40 | 21.50 | 232.32 | 0.4429 | 632.0 | 533.8 | |
| 0.54 | 1.62 | 0.29 | 0.88 | -16.87 | 196.41 | 20.51 | 232.83 | 0.4226 | 742.2 | 609.3 | |
| 30.29 | 121.63 | 16.56 | 66.44 | -17.47 | 196.14 | 20.24 | 231.31 | 0.4246 | 1115.0 | 434.1 | |
| 8.36 | -3.00 | 4.54 | -3.00 | -16.56 | 195.77 | 19.87 | 232.61 | 0.4117 | 1063.7 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -16.60 | 195.27 | 19.37 | 231.87 | 0.4058 | 981.0 | 841.4 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -16.45 | 195.02 | 19.12 | 231.84 | 0.4012 | 876.0 | 747.2 | |
| 1.89 | 3.96 | 1.02 | 2.14 | -16.64 | 194.80 | 18.90 | 231.16 | 0.4003 | 1061.5 | 873.9 | |
| 0.00 | 2.07 | 0.00 | 1.11 | -15.46 | 193.96 | 18.06 | 232.43 | 0.3786 | -821.0 | -559.5 | |
| 6.56 | 122.89 | 3.51 | 65.56 | -15.84 | 193.46 | 17.56 | 230.87 | 0.3759 | -961.4 | -473.9 | |
| 4.23 | -9.00 | 2.26 | -9.00 | -16.03 | 193.31 | 17.42 | 230.24 | 0.3758 | -956.8 | 999999 | |
| 3.60 | -9.00 | 1.92 | -9.00 | -15.56 | 193.17 | 17.28 | 231.03 | 0.3696 | -1190.4 | 999999 | |
| 8.54 | -9.00 | 4.54 | -9.00 | -15.41 | 192.99 | 17.10 | 231.09 | 0.3658 | -1339.9 | 999999 | |
| 8.45 | -9.00 | 4.51 | -9.00 | -16.09 | 193.02 | 17.12 | 229.64 | 0.3729 | -1103.9 | 999999 | |
| 1.17 | -9.00 | 0.62 | -9.00 | -16.28 | 193.04 | 17.14 | 229.27 | 0.3749 | -760.5 | 999999 | |
| 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. | |