SDO HMI 2014-07-05 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.60 | 0.00 | 12.81 | 4.28 | 258.75 | 0.87 | 214.83 | 0.1293 | 910.4 | 705.5 | |
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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 | 2.36 | 0.00 | 1.21 | -3.94 | 270.08 | 12.21 | 239.24 | 0.2466 | 1115.0 | 877.1 | |
| 0.00 | 2.72 | 0.00 | 1.37 | 1.45 | 266.59 | 8.72 | 257.91 | 0.1557 | 660.0 | 527.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 3.91 | 264.52 | 6.64 | 275.01 | 0.1164 | 859.0 | 675.7 | |
| 0.00 | 2.54 | 0.00 | 1.28 | 10.20 | 264.03 | 6.15 | 318.61 | 0.1602 | 899.0 | 744.3 | |
| 0.00 | 2.00 | 0.00 | 0.99 | 2.35 | 260.62 | 2.75 | 249.98 | 0.0512 | 698.0 | 626.2 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 4.54 | 260.26 | 2.39 | 296.66 | 0.0467 | 998.0 | 802.7 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 7.35 | 259.69 | 1.82 | 335.72 | 0.0769 | 837.0 | 628.4 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.14 | 259.66 | 1.79 | 334.90 | 0.0733 | 914.0 | 715.8 | |
| 0.00 | 1.82 | 0.00 | 0.90 | 5.89 | 259.23 | 1.35 | 332.06 | 0.0503 | 1003.0 | 813.3 | |
| 0.00 | 1.73 | 0.00 | 0.86 | 7.80 | 251.60 | -6.28 | 54.27 | 0.1341 | 1032.0 | 777.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 4.23 | 251.02 | -6.86 | 82.47 | 0.1206 | 902.0 | 598.4 | |
| 0.00 | 1.73 | 0.00 | 0.86 | 5.96 | 250.26 | -7.61 | 70.74 | 0.1402 | 946.0 | 617.3 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 3.97 | 248.86 | -9.01 | 85.78 | 0.1574 | 1000.0 | 688.6 | |
| 0.00 | 2.63 | 0.00 | 1.32 | 3.42 | 248.62 | -9.25 | 89.30 | 0.1613 | 882.0 | 739.1 | |
| 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. | |