SDO HMI 2014-03-26 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.14 | 0.00 | 11.00 | -14.20 | 127.12 | -29.38 | 107.21 | 0.4979 | 598.7 | 498.7 | |
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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 | 1.40 | 0.00 | 0.73 | -9.51 | 137.06 | -19.44 | 99.30 | 0.3340 | 680.0 | 564.0 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -14.99 | 132.45 | -24.05 | 111.16 | 0.4238 | 802.0 | 589.1 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -15.58 | 132.07 | -24.43 | 112.23 | 0.4321 | 739.0 | 630.1 | |
| 0.00 | 3.32 | 0.00 | 1.83 | -15.82 | 131.94 | -24.56 | 112.66 | 0.4352 | 731.0 | 612.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -15.17 | 131.68 | -24.82 | 111.06 | 0.4359 | 791.0 | 604.2 | |
| 0.00 | 1.40 | 0.00 | 0.77 | -15.35 | 131.62 | -24.87 | 111.42 | 0.4376 | 687.0 | 537.7 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -13.70 | 130.12 | -26.38 | 106.99 | 0.4533 | 555.0 | 451.7 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -12.96 | 129.31 | -27.19 | 105.07 | 0.4631 | 664.0 | 535.1 | |
| 0.00 | 1.22 | 0.00 | 0.68 | -12.71 | 129.27 | -27.23 | 104.54 | 0.4630 | 702.0 | 573.1 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -20.91 | 124.18 | -32.32 | 117.58 | 0.5656 | 653.0 | 546.2 | |
| 0.00 | 1.57 | 0.00 | 0.92 | -12.31 | 124.41 | -32.09 | 102.35 | 0.5334 | 679.0 | 470.0 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -18.05 | 121.46 | -35.03 | 111.54 | 0.5890 | 564.0 | 498.2 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -9.99 | 118.66 | -37.84 | 97.55 | 0.6117 | 723.0 | 473.8 | |
| 0.00 | 1.57 | 0.00 | 1.00 | -10.03 | 117.13 | -39.37 | 97.54 | 0.6323 | 557.0 | 484.2 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -22.00 | 112.25 | -44.25 | 114.38 | 0.7127 | -546.0 | -450.6 | |
| 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. | |