SDO HMI 2014-09-13 05:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.12 | 38.37 | 9.63 | 56.33 | 13.45 | 348.20 | -71.37 | 78.26 | 0.9406 | -21.4 | 140.7 | |
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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 |
| 0.00 | 1.16 | 0.00 | 1.28 | 14.61 | 355.15 | -64.41 | 77.24 | 0.8967 | -319.0 | -282.8 | |
| 4.98 | 9.44 | 5.87 | 11.14 | 12.48 | 353.50 | -66.07 | 79.56 | 0.9092 | -413.5 | -124.4 | |
| 0.00 | 3.03 | 0.00 | 3.54 | 8.69 | 353.94 | -65.63 | 83.76 | 0.9076 | -398.0 | -320.4 | |
| 0.00 | 2.94 | 0.00 | 3.68 | 12.61 | 351.92 | -67.65 | 79.35 | 0.9201 | 154.0 | 111.3 | |
| 0.00 | 2.40 | 0.00 | 3.72 | 14.34 | 347.08 | -72.49 | 77.26 | 0.9487 | 410.0 | 420.3 | |
| 0.00 | 1.69 | 0.00 | 2.70 | 14.38 | 346.40 | -73.17 | 77.18 | 0.9522 | 355.0 | 292.8 | |
| 0.53 | 3.83 | 0.85 | 5.98 | 14.03 | 346.59 | -72.98 | 77.56 | 0.9514 | 316.0 | 407.0 | |
| 0.36 | 1.60 | 0.59 | 2.66 | 15.00 | 345.62 | -73.95 | 76.48 | 0.9560 | 4.0 | -8.6 | |
| 0.00 | 3.56 | 0.00 | 5.69 | 13.82 | 346.43 | -73.14 | 77.76 | 0.9522 | 191.0 | 146.1 | |
| 0.00 | 1.42 | 0.00 | 2.49 | 14.46 | 344.72 | -74.85 | 77.00 | 0.9605 | 434.0 | 352.1 | |
| 0.00 | 2.85 | 0.00 | 5.13 | 14.41 | 344.28 | -75.29 | 77.02 | 0.9626 | 388.0 | 258.9 | |
| 1.25 | 4.18 | 2.32 | 7.82 | 14.24 | 343.68 | -75.89 | 77.16 | 0.9653 | 206.6 | 144.5 | |
| 0.00 | 0.27 | 0.00 | 0.50 | 13.89 | 343.64 | -75.93 | 77.52 | 0.9656 | 64.0 | 106.7 | |
| 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. | |