SDO HMI 2014-11-28 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.37 | 400.27 | 38.59 | 226.69 | 16.19 | 110.42 | -25.07 | 57.37 | 0.4850 | -929.7 | -326.1 | |
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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 |
| 68.37 | 385.65 | 38.59 | 217.90 | 16.19 | 110.68 | -24.81 | 57.17 | 0.4816 | -1422.6 | -367.5 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 17.21 | 107.03 | -28.46 | 58.61 | 0.5353 | 807.0 | 687.5 | |
| 0.00 | 1.37 | 0.00 | 0.80 | 16.50 | 106.55 | -28.94 | 60.19 | 0.5368 | 468.0 | 366.3 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 15.48 | 105.68 | -29.80 | 62.55 | 0.5419 | 795.0 | 624.4 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 14.81 | 105.29 | -30.19 | 63.97 | 0.5432 | 656.0 | 529.8 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 16.08 | 104.59 | -30.90 | 62.29 | 0.5595 | 682.0 | 491.2 | |
| 0.00 | 0.51 | 0.00 | 0.31 | 17.18 | 104.21 | -31.28 | 60.75 | 0.5707 | 615.0 | 508.8 | |
| 0.00 | 2.22 | 0.00 | 1.34 | 17.03 | 104.09 | -31.39 | 61.08 | 0.5713 | 511.0 | 401.5 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 16.46 | 102.66 | -32.82 | 62.91 | 0.5861 | 763.0 | 580.6 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 16.68 | 102.51 | -32.97 | 62.66 | 0.5892 | 494.0 | 395.8 | |
| 0.00 | 1.03 | 0.00 | 0.63 | 15.93 | 102.06 | -33.42 | 64.10 | 0.5910 | 707.0 | 562.0 | |
| 0.00 | 1.28 | 0.00 | 0.79 | 15.50 | 101.81 | -33.67 | 64.93 | 0.5921 | 733.0 | 637.3 | |
| 0.00 | 1.45 | 0.00 | 0.89 | 15.23 | 101.79 | -33.70 | 65.38 | 0.5911 | 635.0 | 499.5 | |
| 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. | |