SDO HMI 2014-09-22 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.57 | 0.00 | 11.60 | 13.76 | 348.47 | 44.97 | 282.78 | 0.7025 | 108.1 | 129.1 | |
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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 | 1.33 | 0.00 | 1.12 | 10.26 | 357.96 | 54.46 | 277.56 | 0.8099 | -388.0 | -301.9 | |
| 0.00 | 1.24 | 0.00 | 1.01 | 11.96 | 356.85 | 53.35 | 279.67 | 0.7984 | -536.0 | -403.0 | |
| 0.00 | 1.15 | 0.00 | 0.91 | 13.92 | 355.30 | 51.80 | 282.19 | 0.7826 | -591.0 | -500.2 | |
| 0.00 | 0.44 | 0.00 | 0.35 | 14.17 | 354.58 | 51.08 | 282.55 | 0.7751 | -484.0 | -450.8 | |
| 0.00 | 1.68 | 0.00 | 1.25 | 13.87 | 352.26 | 48.76 | 282.28 | 0.7494 | -568.0 | -472.7 | |
| 0.00 | 1.06 | 0.00 | 0.72 | 11.04 | 347.25 | 43.75 | 278.61 | 0.6888 | 553.0 | 406.0 | |
| 0.00 | 1.42 | 0.00 | 0.96 | 12.35 | 346.88 | 43.38 | 280.54 | 0.6847 | 632.0 | 507.3 | |
| 0.00 | 2.57 | 0.00 | 1.69 | 15.69 | 344.65 | 41.15 | 285.78 | 0.6607 | 675.0 | 521.6 | |
| 0.00 | 2.13 | 0.00 | 1.37 | 16.09 | 342.98 | 39.48 | 286.74 | 0.6402 | 765.0 | 646.5 | |
| 0.00 | 2.04 | 0.00 | 1.27 | 13.45 | 341.14 | 37.64 | 282.89 | 0.6116 | 627.0 | 440.2 | |
| 0.00 | 1.51 | 0.00 | 0.95 | 16.51 | 341.59 | 38.09 | 287.72 | 0.6232 | 504.0 | 359.7 | |
| 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. | |