SDO HMI 2014-07-05 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.55 | 24.80 | 0.28 | 12.50 | 7.50 | 260.08 | -2.21 | 164.94 | 0.1698 | 858.3 | 684.9 | |
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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 |
| 0.55 | 2.45 | 0.28 | 1.26 | 6.00 | 276.70 | 14.40 | 281.04 | 0.2532 | 913.7 | 642.1 | |
| 0.00 | 1.64 | 0.00 | 0.82 | 8.47 | 269.44 | 7.14 | 306.17 | 0.1530 | 770.0 | 572.8 | |
| 0.00 | 3.27 | 0.00 | 1.65 | 11.82 | 268.20 | 5.91 | 325.75 | 0.1798 | 1024.0 | 754.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.61 | 266.28 | 3.99 | 323.27 | 0.1155 | 899.0 | 720.6 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 10.22 | 262.49 | 0.20 | 358.40 | 0.1204 | 896.0 | 738.1 | |
| 0.00 | 1.64 | 0.00 | 0.81 | 4.38 | 260.01 | -2.29 | 65.30 | 0.0441 | 910.0 | 700.0 | |
| 0.00 | 2.63 | 0.00 | 1.31 | 7.58 | 259.38 | -2.92 | 34.20 | 0.0901 | 941.0 | 739.4 | |
| 0.00 | 1.73 | 0.00 | 0.86 | 7.64 | 259.17 | -3.13 | 35.73 | 0.0931 | 842.0 | 670.8 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 6.32 | 256.77 | -5.52 | 61.27 | 0.1096 | 844.0 | 707.6 | |
| 0.00 | 2.00 | 0.00 | 1.01 | 7.04 | 250.46 | -11.84 | 72.07 | 0.2150 | 854.0 | 709.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 6.82 | 250.15 | -12.15 | 73.44 | 0.2190 | 827.0 | 620.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 3.79 | 249.08 | -13.22 | 87.61 | 0.2294 | 1014.0 | 835.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 3.82 | 248.73 | -13.56 | 87.54 | 0.2353 | 758.0 | 604.1 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 6.57 | 247.44 | -14.86 | 77.07 | 0.2625 | 586.0 | 499.2 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 7.13 | 245.54 | -16.76 | 76.51 | 0.2955 | 781.0 | 620.7 | |
| 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. | |