SDO HMI 2014-07-16 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 | 16.00 | 0.00 | 11.91 | 9.13 | 163.07 | 48.01 | 278.57 | 0.7389 | 298.9 | 248.0 | |
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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 | 1.36 | 0.00 | 1.21 | 7.01 | 171.49 | 56.42 | 275.46 | 0.8328 | -463.0 | -334.5 | |
| 0.00 | 0.73 | 0.00 | 0.64 | 6.16 | 170.84 | 55.77 | 274.42 | 0.8266 | 394.0 | 315.6 | |
| 0.00 | 0.64 | 0.00 | 0.52 | 4.86 | 168.22 | 53.15 | 272.73 | 0.8005 | -460.0 | -395.6 | |
| 0.00 | 1.09 | 0.00 | 0.91 | 9.02 | 168.87 | 53.80 | 277.93 | 0.8069 | -384.0 | -325.4 | |
| 0.00 | 1.09 | 0.00 | 0.89 | 4.94 | 167.87 | 52.81 | 272.82 | 0.7968 | -273.0 | -360.2 | |
| 0.00 | 2.45 | 0.00 | 2.01 | 12.69 | 167.99 | 52.93 | 282.56 | 0.7996 | 765.0 | 529.3 | |
| 0.00 | 1.36 | 0.00 | 1.07 | 11.53 | 166.19 | 51.12 | 281.24 | 0.7800 | 606.0 | 513.5 | |
| 0.00 | 0.91 | 0.00 | 0.61 | 6.79 | 158.15 | 43.08 | 275.19 | 0.6833 | 357.0 | 261.9 | |
| 0.00 | 0.82 | 0.00 | 0.54 | 9.24 | 156.96 | 41.89 | 278.89 | 0.6694 | 483.0 | 418.9 | |
| 0.00 | 0.91 | 0.00 | 0.60 | 6.43 | 156.28 | 41.22 | 274.68 | 0.6592 | 505.0 | 469.2 | |
| 0.00 | 0.91 | 0.00 | 0.60 | 9.18 | 156.41 | 41.35 | 278.85 | 0.6623 | 641.0 | 585.9 | |
| 0.00 | 0.73 | 0.00 | 0.48 | 8.97 | 156.22 | 41.15 | 278.56 | 0.6596 | 591.0 | 595.8 | |
| 0.00 | 2.18 | 0.00 | 1.34 | 10.77 | 151.46 | 36.39 | 282.11 | 0.5983 | 769.0 | 591.9 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 12.50 | 148.07 | 33.00 | 285.97 | 0.5552 | 654.0 | 548.4 | |
| 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. | |