SDO HMI 2014-07-06 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.09 | 50.51 | 11.81 | 39.25 | -12.72 | 298.21 | 48.05 | 250.36 | 0.7724 | -5.1 | 1.6 | |
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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 |
| 6.54 | 24.62 | 5.20 | 19.56 | -12.91 | 299.24 | 49.08 | 250.47 | 0.7837 | 787.3 | 543.1 | |
| 2.91 | -1.00 | 2.31 | -1.00 | -13.29 | 299.20 | 49.04 | 249.99 | 0.7844 | 752.2 | 999999 | |
| 0.00 | 0.45 | 0.00 | 0.36 | -13.57 | 299.08 | 48.92 | 249.61 | 0.7840 | 612.0 | 545.4 | |
| 0.00 | 0.91 | 0.00 | 0.70 | -13.00 | 297.89 | 47.73 | 249.90 | 0.7701 | -321.0 | -243.2 | |
| 1.36 | 7.54 | 1.04 | 5.74 | -11.84 | 297.38 | 47.22 | 251.19 | 0.7611 | -655.0 | -537.0 | |
| 1.09 | 6.27 | 0.84 | 4.80 | -12.80 | 297.61 | 47.45 | 250.05 | 0.7664 | -501.2 | -292.4 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -13.79 | 297.82 | 47.66 | 248.88 | 0.7717 | -138.0 | -252.0 | |
| 0.00 | 1.00 | 0.00 | 0.78 | -14.11 | 297.81 | 47.65 | 248.49 | 0.7727 | -393.0 | -333.7 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -11.61 | 297.14 | 46.99 | 251.41 | 0.7579 | -461.0 | -383.4 | |
| 1.82 | -6.00 | 1.39 | -6.00 | -12.85 | 297.34 | 47.18 | 249.90 | 0.7638 | -396.8 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.89 | -12.08 | 296.97 | 46.81 | 250.75 | 0.7575 | -460.0 | -409.8 | |
| 0.73 | 1.73 | 0.56 | 1.32 | -13.54 | 297.14 | 46.99 | 248.96 | 0.7639 | -496.1 | -325.1 | |
| 0.00 | 1.54 | 0.00 | 1.16 | -11.93 | 296.53 | 46.37 | 250.79 | 0.7522 | -608.0 | -576.2 | |
| 0.00 | 1.00 | 0.00 | 0.75 | -11.98 | 296.31 | 46.16 | 250.64 | 0.7501 | -732.0 | -623.7 | |
| 0.00 | 0.64 | 0.00 | 0.47 | -11.73 | 296.17 | 46.01 | 250.93 | 0.7477 | -616.0 | -493.6 | |
| 0.64 | 2.18 | 0.47 | 1.62 | -12.20 | 296.14 | 45.98 | 250.31 | 0.7488 | -609.0 | -533.6 | |
| 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. | |