SDO HMI 2014-07-05 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.99 | 0.00 | 9.04 | 6.82 | 263.24 | -0.15 | 154.97 | 0.1590 | 742.3 | 671.6 | |
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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 | 0.64 | 0.00 | 0.33 | 4.22 | 282.83 | 19.44 | 273.26 | 0.3339 | -796.0 | -551.6 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 5.92 | 276.69 | 13.29 | 281.54 | 0.2345 | 894.0 | 734.2 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 9.02 | 269.92 | 6.53 | 311.54 | 0.1507 | 721.0 | 481.2 | |
| 0.00 | 1.73 | 0.00 | 0.86 | -1.87 | 269.31 | 5.92 | 228.74 | 0.1377 | 867.0 | 714.5 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 11.79 | 268.20 | 4.81 | 330.90 | 0.1695 | 982.0 | 827.5 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 8.61 | 266.20 | 2.81 | 332.26 | 0.1046 | 885.0 | 724.0 | |
| 0.00 | 2.27 | 0.00 | 1.13 | 10.18 | 262.53 | -0.86 | 7.07 | 0.1208 | 836.0 | 693.7 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 9.84 | 260.89 | -2.50 | 20.75 | 0.1219 | 1037.0 | 812.4 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 1.42 | 260.06 | -3.33 | 119.80 | 0.0672 | 965.0 | 811.6 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 4.34 | 260.03 | -3.37 | 73.09 | 0.0615 | 834.0 | 742.2 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 7.64 | 259.36 | -4.03 | 42.78 | 0.1030 | 940.0 | 769.2 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 6.93 | 250.58 | -12.82 | 73.73 | 0.2304 | 760.0 | 585.9 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 7.10 | 245.47 | -17.92 | 77.33 | 0.3143 | 725.0 | 626.7 | |
| 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. | |