SDO HMI 2014-09-22 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.40 | 0.00 | 8.84 | -17.67 | 286.08 | -15.22 | 151.19 | 0.4869 | 636.7 | 464.6 | |
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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 | 0.64 | -9.54 | 299.48 | -1.82 | 173.75 | 0.2887 | 866.0 | 678.0 | |
| 0.00 | 1.77 | 0.00 | 0.91 | -8.17 | 297.51 | -3.79 | 166.01 | 0.2718 | 869.0 | 512.8 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -11.62 | 295.37 | -5.93 | 162.44 | 0.3369 | 721.0 | 627.5 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -11.16 | 290.83 | -10.48 | 150.14 | 0.3599 | 725.0 | 644.8 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -15.25 | 287.74 | -13.57 | 148.98 | 0.4410 | 564.0 | 462.0 | |
| 0.00 | 2.21 | 0.00 | 1.28 | -20.69 | 286.79 | -14.51 | 153.11 | 0.5202 | 51.0 | 110.5 | |
| 0.00 | 1.24 | 0.00 | 0.73 | -19.36 | 282.73 | -18.58 | 145.60 | 0.5341 | 705.0 | 531.5 | |
| 0.00 | 2.04 | 0.00 | 1.25 | -23.36 | 281.14 | -20.16 | 147.64 | 0.5935 | 642.0 | 502.9 | |
| 0.00 | 1.33 | 0.00 | 0.82 | -23.13 | 280.79 | -20.51 | 146.98 | 0.5935 | 514.0 | 401.1 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -23.96 | 280.16 | -21.14 | 147.01 | 0.6077 | 539.0 | 507.2 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -24.08 | 279.82 | -21.48 | 146.72 | 0.6116 | 635.0 | 498.5 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -11.75 | 280.77 | -20.54 | 132.51 | 0.4678 | 657.0 | 519.0 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -13.38 | 278.56 | -22.74 | 132.12 | 0.5090 | 789.0 | 532.0 | |
| 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. | |