SDO HMI 2014-09-22 03:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.12 | 0.00 | 9.38 | 7.85 | 333.17 | 31.32 | 273.51 | 0.5156 | 247.0 | 190.4 | |
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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 | 0.62 | 0.00 | 0.41 | 6.28 | 343.84 | 41.99 | 271.51 | 0.6675 | -637.0 | -506.7 | |
| 0.00 | 2.48 | 0.00 | 1.60 | 9.31 | 342.23 | 40.37 | 276.08 | 0.6451 | -657.0 | -518.0 | |
| 0.00 | 0.89 | 0.00 | 0.57 | 11.19 | 341.55 | 39.70 | 279.03 | 0.6368 | -577.0 | -408.8 | |
| 0.00 | 1.06 | 0.00 | 0.66 | 8.24 | 338.92 | 37.07 | 274.31 | 0.6005 | -618.0 | -450.9 | |
| 0.00 | 1.15 | 0.00 | 0.65 | 4.69 | 331.24 | 29.39 | 266.98 | 0.4917 | 586.0 | 570.1 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 3.90 | 330.72 | 28.87 | 265.25 | 0.4853 | 729.0 | 614.3 | |
| 0.00 | 1.86 | 0.00 | 1.04 | 8.24 | 329.87 | 28.02 | 274.26 | 0.4682 | 658.0 | 573.0 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 8.57 | 329.38 | 27.53 | 274.99 | 0.4607 | 696.0 | 587.7 | |
| 0.00 | 1.42 | 0.00 | 0.79 | 7.50 | 329.10 | 27.25 | 272.65 | 0.4563 | 653.0 | 503.4 | |
| 0.00 | 2.13 | 0.00 | 1.18 | 6.59 | 328.60 | 26.74 | 270.60 | 0.4489 | 690.0 | 540.6 | |
| 0.00 | 1.59 | 0.00 | 0.88 | 6.58 | 327.68 | 25.83 | 270.49 | 0.4347 | 711.0 | 513.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.24 | 321.71 | 19.86 | 286.33 | 0.3475 | 730.0 | 476.5 | |
| 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. | |