SDO HMI 2014-09-20 10:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.27 | 0.00 | 9.22 | 8.95 | 331.56 | 7.14 | 269.51 | 0.1525 | 444.6 | 346.8 | |
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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 | 0.66 | 7.11 | 345.11 | 20.69 | 271.33 | 0.3522 | -878.0 | -675.0 | |
| 0.00 | 2.39 | 0.00 | 1.26 | 8.84 | 344.23 | 19.81 | 276.40 | 0.3384 | -782.0 | -548.7 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 9.88 | 339.61 | 15.19 | 281.58 | 0.2647 | -812.0 | -655.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.99 | 330.41 | 5.99 | 288.08 | 0.1090 | 902.0 | 748.7 | |
| 0.00 | 1.51 | 0.00 | 0.75 | 9.41 | 330.08 | 5.66 | 292.85 | 0.1061 | 853.0 | 639.4 | |
| 0.00 | 1.60 | 0.00 | 0.79 | 7.62 | 329.29 | 4.87 | 276.45 | 0.0851 | 833.0 | 611.4 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 7.68 | 328.98 | 4.57 | 277.63 | 0.0800 | 924.0 | 677.6 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 7.68 | 328.77 | 4.35 | 278.00 | 0.0763 | 895.0 | 720.3 | |
| 0.00 | 3.37 | 0.00 | 1.67 | 7.39 | 328.01 | 3.59 | 274.91 | 0.0626 | 876.0 | 755.9 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 8.27 | 327.25 | 2.84 | 292.80 | 0.0534 | 977.0 | 744.8 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 12.44 | 324.46 | 0.04 | 359.55 | 0.0936 | 757.0 | 549.9 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 14.66 | 317.01 | -7.41 | 43.24 | 0.1830 | 790.0 | 677.2 | |
| 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. | |