SDO HMI 2014-09-21 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 |
| 0.00 | 13.46 | 0.00 | 8.90 | 13.96 | 350.64 | 41.07 | 283.85 | 0.6546 | 57.9 | -73.7 | |
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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 | 1.06 | 0.00 | 0.80 | 14.01 | 358.67 | 49.10 | 282.47 | 0.7533 | -421.0 | -309.8 | |
| 0.00 | 1.95 | 0.00 | 1.43 | 11.74 | 357.47 | 47.89 | 279.47 | 0.7387 | -481.0 | -461.1 | |
| 0.00 | 0.80 | 0.00 | 0.58 | 11.89 | 357.09 | 47.52 | 279.69 | 0.7344 | -533.0 | -468.3 | |
| 0.00 | 0.97 | 0.00 | 0.70 | 11.50 | 356.68 | 47.11 | 279.17 | 0.7296 | -548.0 | -520.5 | |
| 0.00 | 0.80 | 0.00 | 0.57 | 12.06 | 356.54 | 46.97 | 279.94 | 0.7280 | -823.0 | -732.4 | |
| 0.00 | 1.86 | 0.00 | 1.24 | 14.33 | 351.87 | 42.30 | 283.57 | 0.6731 | -771.0 | -491.4 | |
| 0.00 | 0.53 | 0.00 | 0.33 | 12.47 | 346.66 | 37.09 | 281.39 | 0.6029 | 613.0 | 528.8 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 15.78 | 344.81 | 35.24 | 287.33 | 0.5838 | 632.0 | 483.1 | |
| 0.00 | 1.24 | 0.00 | 0.74 | 16.23 | 342.77 | 33.20 | 288.76 | 0.5574 | 745.0 | 509.6 | |
| 0.00 | 1.24 | 0.00 | 0.73 | 16.11 | 341.81 | 32.24 | 288.89 | 0.5439 | 800.0 | 647.8 | |
| 0.00 | 1.15 | 0.00 | 0.68 | 16.37 | 341.60 | 32.03 | 289.44 | 0.5418 | 766.0 | 560.5 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 16.24 | 339.67 | 30.10 | 290.02 | 0.5145 | 716.0 | 451.5 | |
| 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. | |