SDO HMI 2014-09-24 13:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.30 | 25.28 | 1.16 | 12.81 | 14.78 | 261.06 | -8.91 | 47.39 | 0.2045 | 186.9 | 306.9 | |
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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 | 1.50 | 0.00 | 0.76 | 14.83 | 263.39 | -6.59 | 38.88 | 0.1774 | -887.0 | -711.1 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 14.37 | 263.18 | -6.79 | 41.47 | 0.1738 | -1101.0 | -759.3 | |
| 0.00 | 2.30 | 0.00 | 1.16 | 14.61 | 262.86 | -7.11 | 41.83 | 0.1804 | -816.0 | -797.0 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 14.73 | 262.36 | -7.62 | 43.32 | 0.1877 | -675.0 | -538.5 | |
| 2.30 | 8.22 | 1.16 | 4.14 | 13.38 | 261.56 | -8.42 | 51.60 | 0.1825 | 1035.7 | 869.3 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 15.03 | 260.43 | -9.55 | 48.50 | 0.2149 | -487.0 | -301.5 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 15.32 | 260.00 | -9.97 | 48.65 | 0.2235 | 814.0 | 625.4 | |
| 0.00 | 2.03 | 0.00 | 1.04 | 16.72 | 259.81 | -10.17 | 44.65 | 0.2417 | 692.0 | 580.5 | |
| 0.00 | 2.39 | 0.00 | 1.22 | 15.56 | 259.68 | -10.30 | 48.72 | 0.2302 | 1030.0 | 785.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 15.77 | 259.38 | -10.60 | 48.81 | 0.2362 | 876.0 | 724.9 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 15.67 | 259.10 | -10.88 | 49.84 | 0.2388 | 890.0 | 714.0 | |
| 0.00 | 2.30 | 0.00 | 1.18 | 16.46 | 259.02 | -10.95 | 47.50 | 0.2482 | 735.0 | 612.7 | |
| 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. | |