SDO HMI 2014-07-02 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.54 | 19.34 | 0.50 | 12.30 | 5.97 | 269.41 | -37.53 | 84.13 | 0.5991 | -252.2 | -250.3 | |
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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 | 1.45 | 0.00 | 0.81 | 4.70 | 279.07 | -27.87 | 85.54 | 0.4692 | -1001.0 | -816.2 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 4.21 | 278.78 | -28.16 | 86.62 | 0.4734 | -682.0 | -572.6 | |
| 0.00 | 3.81 | 0.00 | 2.14 | 4.73 | 278.72 | -28.22 | 85.53 | 0.4746 | -794.0 | -744.9 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 4.60 | 278.59 | -28.35 | 85.80 | 0.4765 | -740.0 | -655.5 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 4.84 | 278.40 | -28.54 | 85.32 | 0.4795 | -646.0 | -634.0 | |
| 0.00 | 2.09 | 0.00 | 1.18 | 6.48 | 278.11 | -28.83 | 81.95 | 0.4859 | -716.0 | -556.7 | |
| 0.00 | 2.09 | 0.00 | 1.21 | 5.48 | 275.86 | -31.08 | 84.30 | 0.5184 | -736.0 | -651.9 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 3.36 | 275.35 | -31.59 | 88.40 | 0.5252 | 603.0 | 385.1 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 1.89 | 272.84 | -34.09 | 91.01 | 0.5625 | -607.0 | -611.8 | |
| 0.00 | 0.91 | 0.00 | 0.63 | 7.91 | 262.24 | -44.70 | 81.75 | 0.7063 | 509.0 | 456.0 | |
| 0.00 | 2.45 | 0.00 | 1.77 | 9.11 | 260.51 | -46.43 | 80.25 | 0.7282 | 409.0 | 342.5 | |
| 0.00 | 1.00 | 0.00 | 0.87 | 7.66 | 251.63 | -55.31 | 82.73 | 0.8237 | 450.0 | 415.5 | |
| 0.54 | 1.54 | 0.50 | 1.41 | 5.93 | 249.77 | -57.17 | 84.86 | 0.8413 | 364.3 | 309.9 | |
| 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. | |