SDO HMI 2014-07-06 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.00 | 0.00 | 9.59 | 4.48 | 256.60 | 8.09 | 293.81 | 0.1616 | 774.2 | 660.4 | |
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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 | 1.18 | 0.00 | 0.63 | -1.09 | 268.81 | 20.30 | 257.75 | 0.3564 | 869.0 | 686.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 7.16 | 266.86 | 18.35 | 282.26 | 0.3211 | 824.0 | 666.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -3.44 | 263.83 | 15.32 | 245.95 | 0.2901 | 804.0 | 625.2 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 6.34 | 263.02 | 14.51 | 281.91 | 0.2557 | 720.0 | 525.5 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 2.32 | 261.06 | 12.55 | 265.21 | 0.2188 | 803.0 | 615.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 8.00 | 260.30 | 11.79 | 291.76 | 0.2188 | 864.0 | 693.9 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 5.49 | 258.52 | 10.01 | 281.96 | 0.1776 | 861.0 | 684.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | -3.20 | 257.24 | 8.73 | 232.82 | 0.1910 | 830.0 | 591.7 | |
| 0.00 | 1.64 | 0.00 | 0.81 | 7.77 | 251.44 | 2.93 | 326.17 | 0.0914 | 975.0 | 699.3 | |
| 0.00 | 4.82 | 0.00 | 2.39 | 7.68 | 251.13 | 2.62 | 328.50 | 0.0872 | 730.0 | 755.3 | |
| 0.00 | 0.64 | 0.00 | 0.32 | 6.46 | 250.24 | 1.73 | 330.46 | 0.0609 | 340.0 | 480.7 | |
| 0.00 | 2.45 | 0.00 | 1.22 | 3.57 | 248.70 | 0.19 | 305.01 | 0.0040 | 670.0 | 632.9 | |
| 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. | |