SDO HMI 2014-07-19 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.70 | 47.63 | 6.69 | 27.36 | -21.91 | 67.59 | -14.92 | 151.82 | 0.5075 | 148.8 | -36.7 | |
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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 |
| 2.00 | 7.44 | 1.14 | 4.24 | -21.85 | 68.80 | -13.71 | 153.68 | 0.4981 | 899.5 | 882.5 | |
| 2.45 | -1.00 | 1.40 | -1.00 | -21.68 | 68.75 | -13.76 | 153.43 | 0.4962 | 1152.3 | 999999 | |
| 0.45 | 18.33 | 0.26 | 10.48 | -22.10 | 68.57 | -13.94 | 153.54 | 0.5029 | 892.6 | 603.2 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -21.52 | 68.63 | -13.88 | 153.07 | 0.4948 | 1027.0 | 783.9 | |
| 4.08 | -3.00 | 2.34 | -3.00 | -22.03 | 68.41 | -14.10 | 153.21 | 0.5031 | 761.9 | 999999 | |
| 2.27 | -3.00 | 1.29 | -3.00 | -21.55 | 68.39 | -14.12 | 152.72 | 0.4969 | 916.0 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.99 | -21.80 | 68.13 | -14.38 | 152.53 | 0.5020 | 481.0 | 425.3 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -22.23 | 67.13 | -15.38 | 151.38 | 0.5146 | -734.0 | -585.5 | |
| 0.45 | 3.54 | 0.26 | 2.04 | -22.00 | 66.61 | -15.90 | 150.35 | 0.5155 | -848.4 | -545.0 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -21.87 | 66.56 | -15.95 | 150.13 | 0.5142 | -964.0 | -713.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -21.83 | 66.42 | -16.09 | 149.89 | 0.5148 | -827.0 | -733.8 | |
| 0.00 | 4.45 | 0.00 | 2.58 | -22.08 | 66.02 | -16.49 | 149.54 | 0.5210 | -766.0 | -748.7 | |
| 0.00 | 4.35 | 0.00 | 2.52 | -21.78 | 65.95 | -16.56 | 149.12 | 0.5177 | -952.0 | -885.0 | |
| 0.00 | 2.81 | 0.00 | 1.64 | -22.33 | 65.61 | -16.90 | 149.19 | 0.5272 | -441.0 | -433.9 | |
| 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. | |