SDO HMI 2014-04-07 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.52 | 0.00 | 11.78 | -8.73 | 7.73 | 7.90 | 247.95 | 0.1530 | 225.7 | 47.2 | |
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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 | 1.59 | 0.00 | 0.80 | -5.92 | 11.97 | 12.14 | 270.52 | 0.2101 | 865.0 | 710.0 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -6.43 | 11.89 | 12.06 | 268.07 | 0.2086 | 628.0 | 427.1 | |
| 0.00 | 1.59 | 0.00 | 0.80 | -7.90 | 11.74 | 11.91 | 260.93 | 0.2079 | 757.0 | 648.1 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -10.86 | 11.19 | 11.35 | 246.53 | 0.2117 | -860.0 | -698.3 | |
| 0.00 | 2.03 | 0.00 | 1.02 | -9.03 | 10.75 | 10.92 | 254.47 | 0.1951 | 718.0 | 691.3 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -9.28 | 10.48 | 10.65 | 252.88 | 0.1917 | 822.0 | 624.6 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -9.20 | 10.17 | 10.34 | 252.87 | 0.1862 | 1026.0 | 771.4 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -10.90 | 8.89 | 9.06 | 241.51 | 0.1767 | 767.0 | 514.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -10.45 | 8.57 | 8.74 | 243.02 | 0.1684 | 846.0 | 700.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -10.04 | 8.16 | 8.32 | 244.27 | 0.1590 | 882.0 | 576.5 | |
| 0.00 | 2.03 | 0.00 | 1.01 | -7.09 | 5.81 | 5.98 | 260.76 | 0.1052 | -1146.0 | -975.4 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -7.82 | 5.61 | 5.77 | 253.58 | 0.1044 | -800.0 | -613.3 | |
| 0.00 | 4.14 | 0.00 | 2.06 | -7.64 | 5.42 | 5.59 | 254.80 | 0.1005 | -1266.0 | -976.2 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -7.56 | 3.57 | 3.74 | 249.14 | 0.0694 | -863.0 | -604.4 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -12.59 | 358.86 | -0.98 | 171.53 | 0.1137 | 1009.0 | 721.5 | |
| 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. | |