SDO HMI 2014-07-05 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.06 | 138.28 | 25.13 | 112.91 | 6.35 | 203.52 | -52.69 | 84.58 | 0.7961 | -664.4 | -193.4 | |
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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 |
| 4.18 | 15.07 | 3.32 | 12.00 | 6.62 | 204.56 | -51.65 | 84.22 | 0.7852 | -940.0 | -562.6 | |
| 1.91 | -1.00 | 1.52 | -1.00 | 6.80 | 204.49 | -51.72 | 83.99 | 0.7860 | -711.1 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.65 | 7.01 | 204.45 | -51.76 | 83.72 | 0.7864 | -270.0 | -242.3 | |
| 0.00 | 0.73 | 0.00 | 0.58 | 6.28 | 204.56 | -51.65 | 84.65 | 0.7852 | -500.0 | -428.4 | |
| 0.00 | 1.45 | 0.00 | 1.16 | 6.42 | 204.24 | -51.97 | 84.48 | 0.7886 | -741.0 | -586.1 | |
| 0.00 | 0.27 | 0.00 | 0.22 | 7.10 | 203.58 | -52.63 | 83.64 | 0.7957 | -347.0 | -388.7 | |
| 23.06 | 110.59 | 18.72 | 90.09 | 6.15 | 203.67 | -52.53 | 84.83 | 0.7946 | -921.9 | -179.0 | |
| 0.00 | 1.18 | 0.00 | 0.97 | 7.33 | 203.29 | -52.92 | 83.35 | 0.7988 | -491.0 | -392.2 | |
| 0.00 | 1.45 | 0.00 | 1.20 | 8.09 | 203.15 | -53.06 | 82.40 | 0.8005 | -540.0 | -394.9 | |
| 1.91 | -7.00 | 1.57 | -7.00 | 6.95 | 203.15 | -53.06 | 83.83 | 0.8003 | -546.6 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.05 | 7.20 | 203.05 | -53.15 | 83.53 | 0.8012 | -306.0 | -237.9 | |
| 0.00 | 0.82 | 0.00 | 0.68 | 6.91 | 202.79 | -53.42 | 83.89 | 0.8039 | 235.0 | 210.6 | |
| 0.00 | 1.09 | 0.00 | 1.00 | 6.96 | 198.64 | -57.57 | 83.89 | 0.8447 | 417.0 | 428.8 | |
| 0.00 | 2.27 | 0.00 | 2.10 | 7.16 | 198.42 | -57.79 | 83.65 | 0.8467 | 548.0 | 445.0 | |
| 0.00 | 1.27 | 0.00 | 1.21 | 7.18 | 197.54 | -58.67 | 83.64 | 0.8548 | 307.0 | 261.2 | |
| 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. | |