SDO HMI 2014-07-05 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.72 | 0.00 | 10.48 | 6.31 | 258.77 | -1.88 | 154.92 | 0.1889 | 749.4 | 586.7 | |
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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 | 1.73 | 0.00 | 0.92 | 4.26 | 282.94 | 22.29 | 273.09 | 0.3804 | -710.0 | -523.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 6.00 | 276.73 | 16.09 | 280.03 | 0.2811 | 864.0 | 757.9 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 8.66 | 266.30 | 5.66 | 313.69 | 0.1354 | 716.0 | 606.5 | |
| 0.00 | 1.00 | 0.00 | 0.50 | -0.02 | 264.73 | 4.08 | 230.63 | 0.0925 | 842.0 | 634.9 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 10.12 | 264.03 | 3.38 | 333.80 | 0.1323 | 994.0 | 700.7 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 10.24 | 262.76 | 2.12 | 343.20 | 0.1262 | 750.0 | 517.0 | |
| 0.00 | 2.27 | 0.00 | 1.13 | 7.52 | 259.45 | -1.19 | 15.78 | 0.0762 | 957.0 | 841.1 | |
| 0.00 | 1.82 | 0.00 | 0.91 | 7.80 | 251.60 | -9.04 | 63.24 | 0.1752 | 1024.0 | 825.1 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 3.95 | 250.92 | -9.73 | 86.08 | 0.1697 | 727.0 | 475.6 | |
| 0.00 | 1.64 | 0.00 | 0.82 | 7.06 | 250.37 | -10.27 | 69.61 | 0.1897 | 881.0 | 704.3 | |
| 0.00 | 2.00 | 0.00 | 1.01 | 6.02 | 250.21 | -10.44 | 75.17 | 0.1873 | 953.0 | 725.7 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 3.44 | 248.81 | -11.84 | 89.14 | 0.2057 | 943.0 | 701.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 7.12 | 245.62 | -15.03 | 75.19 | 0.2673 | 801.0 | 575.5 | |
| 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. | |