SDO HMI 2014-07-13 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 |
| 45.97 | 294.59 | 157.55 | 1022.13 | -7.33 | 241.62 | 81.36 | 261.98 | 0.9890 | -133.8 | 91.0 | |
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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 | 138.48 | 11.62 | 675.13 | -6.67 | 244.26 | 84.01 | 262.88 | 0.9959 | -375.2 | 178.3 | |
| 14.53 | -1.00 | 70.99 | -1.00 | -7.39 | 243.91 | 83.66 | 262.14 | 0.9954 | 71.3 | 999999 | |
| 4.00 | -1.00 | 21.03 | -1.00 | -8.86 | 244.13 | 83.87 | 260.68 | 0.9960 | -80.8 | 999999 | |
| 0.00 | 6.27 | 0.00 | 19.22 | -4.80 | 240.54 | 80.28 | 264.44 | 0.9876 | 349.0 | 214.4 | |
| 0.00 | 1.00 | 0.00 | 2.43 | -4.47 | 238.08 | 77.83 | 264.56 | 0.9799 | -115.0 | -51.5 | |
| 0.00 | 4.18 | 0.00 | 9.90 | -4.85 | 237.78 | 77.53 | 264.15 | 0.9789 | -287.0 | -184.8 | |
| 5.09 | 56.39 | 12.10 | 127.85 | -6.57 | 237.70 | 77.44 | 262.38 | 0.9792 | -315.0 | 77.0 | |
| 0.00 | 1.00 | 0.00 | 2.16 | -6.41 | 236.39 | 76.13 | 262.41 | 0.9743 | -328.0 | -251.0 | |
| 12.17 | 62.57 | 27.99 | 143.66 | -7.95 | 237.07 | 76.81 | 260.92 | 0.9775 | -365.9 | -215.5 | |
| 6.36 | 21.88 | 10.79 | 37.09 | -4.95 | 232.75 | 72.49 | 263.53 | 0.9575 | -439.6 | -308.1 | |
| 1.82 | 2.82 | 3.03 | 4.69 | -5.66 | 232.34 | 72.09 | 262.75 | 0.9558 | -473.4 | -409.2 | |
| 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. | |