SDO HMI 2014-08-01 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.26 | 0.00 | 13.34 | 13.00 | 258.76 | -7.94 | 190.96 | 0.2150 | 382.1 | 218.9 | |
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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 |
| 0.00 | 3.89 | 0.00 | 1.96 | 16.13 | 267.51 | 0.81 | 355.66 | 0.1808 | -954.0 | -572.5 | |
| 0.00 | 2.08 | 0.00 | 1.05 | 15.70 | 267.13 | 0.43 | 357.59 | 0.1730 | -878.0 | -677.5 | |
| 0.00 | 2.26 | 0.00 | 1.16 | 18.47 | 260.81 | -5.89 | 23.86 | 0.2416 | -665.0 | -449.0 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 9.76 | 260.37 | -6.33 | 57.30 | 0.1297 | 894.0 | 674.1 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 6.49 | 259.89 | -6.80 | 83.73 | 0.1190 | 141.0 | 106.2 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 22.54 | 258.27 | -8.43 | 25.11 | 0.3207 | -665.0 | -392.2 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 16.15 | 258.42 | -8.27 | 37.41 | 0.2286 | 1054.0 | 870.0 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 9.61 | 258.44 | -8.25 | 64.46 | 0.1576 | 994.0 | 751.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 11.97 | 256.55 | -10.15 | 57.66 | 0.2049 | 775.0 | 610.0 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 4.37 | 255.87 | -10.83 | 97.03 | 0.1896 | 1003.0 | 786.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 4.70 | 255.59 | -11.11 | 95.13 | 0.1938 | 901.0 | 802.0 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 4.42 | 255.50 | -11.20 | 96.49 | 0.1958 | 893.0 | 589.9 | |
| 0.00 | 3.53 | 0.00 | 1.80 | 13.14 | 254.92 | -11.78 | 56.85 | 0.2386 | 719.0 | 443.3 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 18.68 | 249.88 | -16.82 | 50.36 | 0.3576 | 725.0 | 568.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 14.33 | 248.54 | -18.15 | 63.07 | 0.3401 | 795.0 | 542.8 | |
| 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. | |