SDO HMI 2014-09-07 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.57 | 40.71 | 15.90 | 48.61 | -20.68 | 79.02 | -60.32 | 116.73 | 0.9110 | 41.6 | -59.2 | |
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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 |
| 0.62 | 2.50 | 0.67 | 2.68 | -20.52 | 82.45 | -56.89 | 117.73 | 0.8882 | 687.7 | 578.3 | |
| 0.00 | 0.27 | 0.00 | 0.29 | -20.74 | 82.33 | -57.02 | 117.91 | 0.8897 | 383.0 | 436.0 | |
| 0.89 | 1.87 | 0.97 | 2.03 | -20.22 | 81.85 | -57.50 | 117.19 | 0.8916 | 517.8 | 415.4 | |
| 1.16 | 2.77 | 1.27 | 3.03 | -20.47 | 81.70 | -57.64 | 117.40 | 0.8933 | 333.5 | 244.4 | |
| 0.00 | 1.07 | 0.00 | 1.20 | -20.72 | 81.00 | -58.35 | 117.41 | 0.8987 | 148.0 | 79.6 | |
| 0.00 | 0.62 | 0.00 | 0.73 | -21.68 | 80.25 | -59.09 | 118.15 | 0.9061 | 94.0 | 105.3 | |
| 1.70 | 4.91 | 1.98 | 5.74 | -21.53 | 80.10 | -59.25 | 117.94 | 0.9067 | 515.5 | 278.7 | |
| 4.11 | 5.54 | 4.80 | 6.46 | -21.18 | 79.88 | -59.46 | 117.51 | 0.9073 | 290.1 | 138.7 | |
| 0.00 | 0.45 | 0.00 | 0.49 | -19.08 | 80.81 | -58.54 | 115.61 | 0.8959 | 478.0 | 456.4 | |
| 0.00 | 1.16 | 0.00 | 1.35 | -19.83 | 79.40 | -59.94 | 115.94 | 0.9072 | -548.0 | -535.8 | |
| 0.00 | 1.87 | 0.00 | 2.24 | -20.29 | 78.84 | -60.51 | 116.24 | 0.9119 | -536.0 | -455.8 | |
| 5.09 | 13.84 | 6.21 | 16.81 | -20.07 | 78.19 | -61.15 | 115.80 | 0.9155 | -419.2 | -357.8 | |
| 0.00 | 1.07 | 0.00 | 1.35 | -19.87 | 77.30 | -62.04 | 115.31 | 0.9206 | -394.0 | -338.2 | |
| 0.00 | 0.45 | 0.00 | 0.68 | -22.65 | 73.42 | -65.93 | 117.01 | 0.9472 | 170.0 | 113.8 | |
| 0.00 | 2.32 | 0.00 | 3.53 | -22.37 | 73.43 | -65.92 | 116.74 | 0.9467 | 44.0 | 41.3 | |
| 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. | |