SDO HMI 2014-07-09 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.08 | 0.00 | 9.37 | -22.01 | 196.58 | -18.27 | 146.64 | 0.5266 | -29.5 | 31.6 | |
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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 | 1.09 | 0.00 | 0.61 | -21.64 | 203.20 | -11.65 | 156.27 | 0.4681 | 932.0 | 865.9 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.87 | 203.01 | -11.83 | 156.15 | 0.4726 | 801.0 | 660.0 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -22.25 | 202.98 | -11.87 | 156.44 | 0.4780 | 713.0 | 513.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.67 | 202.86 | -11.98 | 155.70 | 0.4707 | 903.0 | 691.2 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -27.11 | 200.31 | -14.54 | 156.36 | 0.5593 | -903.0 | -762.7 | |
| 0.00 | 2.81 | 0.00 | 1.62 | -22.68 | 199.06 | -15.78 | 150.42 | 0.5104 | 839.0 | 649.2 | |
| 0.00 | 0.82 | 0.00 | 0.47 | -22.72 | 198.85 | -16.00 | 150.14 | 0.5125 | 406.0 | 456.8 | |
| 0.00 | 0.82 | 0.00 | 0.47 | -20.51 | 196.17 | -18.67 | 143.62 | 0.5075 | -647.0 | -550.9 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -20.15 | 195.91 | -18.94 | 142.78 | 0.5057 | -766.0 | -543.5 | |
| 0.00 | 0.64 | 0.00 | 0.37 | -20.43 | 195.32 | -19.52 | 142.31 | 0.5143 | -664.0 | -521.7 | |
| 0.00 | 2.18 | 0.00 | 1.30 | -22.41 | 192.74 | -22.10 | 141.40 | 0.5597 | -725.0 | -576.6 | |
| 0.00 | 0.91 | 0.00 | 0.61 | -29.38 | 186.27 | -28.58 | 142.29 | 0.6837 | -597.0 | -504.1 | |
| 0.00 | 1.63 | 0.00 | 0.98 | -16.40 | 186.23 | -28.62 | 126.19 | 0.5714 | -675.0 | -506.4 | |
| 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. | |