SDO HMI 2014-09-13 22:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.38 | 78.41 | 13.08 | 43.82 | -15.73 | 65.83 | 15.61 | 213.87 | 0.4668 | 749.6 | 472.7 | |
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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 | 1.16 | 0.00 | 0.66 | -16.94 | 67.00 | 16.78 | 214.33 | 0.4917 | 536.0 | 321.2 | |
| 3.02 | 4.71 | 1.70 | 2.65 | -15.82 | 66.83 | 16.62 | 215.45 | 0.4764 | 847.8 | 594.0 | |
| 0.00 | 0.98 | 0.00 | 0.55 | -16.44 | 66.85 | 16.64 | 214.71 | 0.4843 | 653.0 | 451.2 | |
| 1.33 | 2.58 | 0.75 | 1.45 | -15.84 | 66.44 | 16.23 | 214.79 | 0.4732 | 849.5 | 722.4 | |
| 6.49 | 61.70 | 3.63 | 34.43 | -15.63 | 66.16 | 15.95 | 214.58 | 0.4682 | 942.7 | 533.0 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -16.29 | 66.15 | 15.94 | 213.76 | 0.4763 | 773.0 | 627.4 | |
| 5.16 | -5.00 | 2.88 | -5.00 | -15.49 | 66.02 | 15.81 | 214.52 | 0.4652 | 1096.4 | 999999 | |
| 7.38 | -5.00 | 4.12 | -5.00 | -15.42 | 65.79 | 15.58 | 214.22 | 0.4622 | 1156.4 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -16.60 | 65.82 | 15.61 | 212.82 | 0.4775 | 601.0 | 532.6 | |
| 0.00 | 2.40 | 0.00 | 1.36 | -18.27 | 64.12 | 13.91 | 208.13 | 0.4861 | 647.0 | 504.8 | |
| 0.00 | 2.04 | 0.00 | 1.13 | -16.90 | 61.76 | 11.54 | 205.23 | 0.4511 | -873.0 | -667.7 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -16.59 | 58.70 | 8.49 | 199.36 | 0.4285 | -708.0 | -544.7 | |
| 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. | |