SDO HMI 2014-07-04 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.71 | 0.00 | 10.23 | 7.76 | 258.65 | -14.68 | 73.93 | 0.2763 | 654.6 | 577.8 | |
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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 | 0.73 | 0.00 | 0.36 | 3.99 | 276.26 | 2.93 | 284.67 | 0.0530 | -878.0 | -637.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.86 | 268.01 | -5.32 | 31.13 | 0.1763 | 882.0 | 735.7 | |
| 0.00 | 1.82 | 0.00 | 0.91 | 6.65 | 267.87 | -5.46 | 57.69 | 0.1124 | 803.0 | 628.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 12.07 | 266.59 | -6.73 | 36.68 | 0.1928 | 806.0 | 699.6 | |
| 0.00 | 2.45 | 0.00 | 1.23 | 9.94 | 266.11 | -7.22 | 46.54 | 0.1713 | 755.0 | 519.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 8.38 | 262.49 | -10.84 | 63.99 | 0.2079 | 738.0 | 594.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 9.20 | 261.84 | -11.49 | 61.86 | 0.2240 | 775.0 | 664.2 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 7.28 | 259.12 | -14.21 | 73.47 | 0.2551 | 970.0 | 756.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 8.44 | 251.59 | -21.74 | 75.50 | 0.3800 | 799.0 | 623.0 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 8.59 | 251.38 | -21.95 | 75.23 | 0.3838 | 804.0 | 597.0 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 8.27 | 250.57 | -22.76 | 76.47 | 0.3954 | 633.0 | 550.8 | |
| 0.00 | 0.64 | 0.00 | 0.34 | 6.06 | 250.55 | -22.78 | 82.04 | 0.3904 | 617.0 | 501.4 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 6.67 | 250.09 | -23.24 | 80.66 | 0.3989 | 639.0 | 470.3 | |
| 0.00 | 3.18 | 0.00 | 1.73 | 4.45 | 249.17 | -24.15 | 86.33 | 0.4105 | 822.0 | 675.6 | |
| 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. | |