SDO HMI 2014-09-22 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.40 | 0.00 | 11.15 | 7.64 | 330.02 | 29.81 | 273.57 | 0.4930 | 346.0 | 350.5 | |
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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 | 1.24 | 0.00 | 0.86 | 8.25 | 345.22 | 45.01 | 274.61 | 0.7045 | -499.0 | -423.8 | |
| 0.00 | 0.80 | 0.00 | 0.55 | 3.19 | 343.99 | 43.78 | 267.23 | 0.6940 | -582.0 | -474.2 | |
| 0.00 | 0.97 | 0.00 | 0.65 | 9.38 | 342.31 | 42.10 | 276.19 | 0.6677 | -674.0 | -555.6 | |
| 0.00 | 1.06 | 0.00 | 0.61 | 3.85 | 330.71 | 30.51 | 265.60 | 0.5100 | 681.0 | 570.0 | |
| 0.00 | 0.44 | 0.00 | 0.25 | 8.30 | 330.54 | 30.33 | 274.38 | 0.5032 | 736.0 | 645.4 | |
| 0.00 | 1.24 | 0.00 | 0.71 | 8.10 | 329.93 | 29.72 | 273.98 | 0.4940 | 677.0 | 529.6 | |
| 0.00 | 1.95 | 0.00 | 1.10 | 6.99 | 328.70 | 28.49 | 271.65 | 0.4756 | 808.0 | 669.4 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 5.53 | 328.40 | 28.19 | 268.53 | 0.4723 | 529.0 | 523.7 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 6.28 | 328.06 | 27.86 | 270.06 | 0.4664 | 742.0 | 598.6 | |
| 0.00 | 3.81 | 0.00 | 2.12 | 6.48 | 327.70 | 27.49 | 270.46 | 0.4606 | 763.0 | 613.1 | |
| 0.00 | 3.10 | 0.00 | 1.69 | 8.38 | 324.81 | 24.61 | 274.75 | 0.4151 | 196.0 | 262.2 | |
| 0.00 | 2.66 | 0.00 | 1.42 | 12.25 | 321.66 | 21.45 | 285.47 | 0.3724 | 775.0 | 599.9 | |
| 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. | |