SDO HMI 2014-07-19 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.33 | 67.97 | 11.53 | 38.75 | -21.81 | 67.57 | -13.29 | 154.40 | 0.4953 | 162.6 | -157.1 | |
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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 |
| 1.09 | 38.66 | 0.62 | 21.90 | -21.84 | 69.03 | -11.83 | 156.86 | 0.4862 | 831.3 | 549.6 | |
| 2.90 | -1.00 | 1.64 | -1.00 | -21.63 | 69.01 | -11.85 | 156.65 | 0.4834 | 1098.4 | 999999 | |
| 7.99 | -1.00 | 4.53 | -1.00 | -21.84 | 68.66 | -12.20 | 156.23 | 0.4885 | 899.1 | 999999 | |
| 6.44 | -1.00 | 3.64 | -1.00 | -21.50 | 68.62 | -12.24 | 155.86 | 0.4841 | 1030.7 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -22.25 | 67.17 | -13.69 | 154.10 | 0.5035 | -704.0 | -481.6 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -22.11 | 66.91 | -13.95 | 153.56 | 0.5034 | -664.0 | -572.5 | |
| 0.00 | 2.18 | 0.00 | 1.25 | -22.05 | 66.72 | -14.14 | 153.18 | 0.5039 | -789.0 | -605.5 | |
| 0.00 | 2.81 | 0.00 | 1.61 | -21.82 | 66.54 | -14.32 | 152.66 | 0.5020 | -959.0 | -791.2 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -21.82 | 66.27 | -14.59 | 152.23 | 0.5040 | -907.0 | -826.4 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -22.31 | 65.98 | -14.88 | 152.25 | 0.5124 | -542.0 | -472.1 | |
| 0.64 | 4.90 | 0.37 | 2.83 | -22.31 | 65.80 | -15.05 | 151.98 | 0.5136 | -797.3 | -608.0 | |
| 1.27 | 12.89 | 0.73 | 7.40 | -21.76 | 65.83 | -15.03 | 151.48 | 0.5063 | -926.8 | -727.8 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -22.35 | 65.46 | -15.40 | 151.49 | 0.5166 | -633.0 | -499.2 | |
| 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. | |