SDO HMI 2014-09-22 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.60 | 0.00 | 10.31 | -16.00 | 287.62 | -11.49 | 155.10 | 0.4358 | 662.5 | 507.9 | |
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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 | 0.97 | 0.00 | 0.51 | -10.53 | 299.86 | 0.75 | 182.42 | 0.3036 | 749.0 | 526.4 | |
| 0.00 | 1.42 | 0.00 | 0.75 | -13.11 | 295.69 | -3.42 | 170.41 | 0.3509 | 811.0 | 686.1 | |
| 0.00 | 2.57 | 0.00 | 1.32 | -5.65 | 291.88 | -7.23 | 150.22 | 0.2533 | 574.0 | 729.1 | |
| 0.00 | 1.51 | 0.00 | 0.79 | -10.90 | 291.50 | -7.61 | 157.04 | 0.3350 | 814.0 | 658.9 | |
| 0.00 | 4.16 | 0.00 | 2.29 | -17.10 | 289.37 | -9.74 | 158.35 | 0.4402 | 224.0 | 249.4 | |
| 0.00 | 1.59 | 0.00 | 0.87 | -14.33 | 285.45 | -13.67 | 147.63 | 0.4294 | 604.0 | 582.1 | |
| 0.00 | 1.68 | 0.00 | 0.97 | -19.36 | 282.65 | -16.47 | 148.71 | 0.5169 | 665.0 | 499.8 | |
| 0.00 | 0.89 | 0.00 | 0.52 | -21.58 | 282.26 | -16.85 | 150.38 | 0.5476 | 741.0 | 574.2 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -18.85 | 281.77 | -17.35 | 146.82 | 0.5176 | 800.0 | 655.0 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -23.38 | 281.06 | -18.05 | 150.42 | 0.5783 | 681.0 | 539.8 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -23.18 | 280.92 | -18.19 | 150.04 | 0.5768 | 641.0 | 369.0 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -24.16 | 280.12 | -19.00 | 149.88 | 0.5942 | 646.0 | 472.3 | |
| 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. | |