SDO HMI 2014-07-09 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.98 | 0.00 | 12.63 | -19.25 | 227.31 | 15.21 | 211.08 | 0.5061 | -168.2 | -17.3 | |
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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 | 0.82 | 0.00 | 0.50 | -15.89 | 242.76 | 30.66 | 236.29 | 0.5918 | 579.0 | 470.1 | |
| 0.00 | 1.09 | 0.00 | 0.66 | -16.58 | 241.11 | 29.02 | 233.87 | 0.5777 | 601.0 | 447.3 | |
| 0.00 | 4.45 | 0.00 | 2.64 | -15.38 | 239.88 | 27.78 | 234.53 | 0.5539 | 694.0 | 713.2 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -13.99 | 237.72 | 25.62 | 234.59 | 0.5169 | 538.0 | 546.3 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -16.14 | 236.49 | 24.39 | 229.86 | 0.5209 | 875.0 | 667.2 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -15.10 | 236.22 | 24.12 | 231.18 | 0.5084 | 561.0 | 486.1 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -17.14 | 232.65 | 20.55 | 223.58 | 0.4885 | -702.0 | -592.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -19.65 | 227.24 | 15.14 | 211.92 | 0.4671 | -534.0 | -494.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -17.42 | 223.98 | 11.89 | 208.65 | 0.4116 | -742.0 | -614.5 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -19.75 | 220.23 | 8.13 | 198.50 | 0.4213 | -774.0 | -483.1 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.03 | 216.98 | 4.88 | 190.29 | 0.4435 | -664.0 | -545.8 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -22.40 | 215.73 | 3.64 | 187.58 | 0.4461 | -699.0 | -483.0 | |
| 0.00 | 1.82 | 0.00 | 1.02 | -23.76 | 213.87 | 1.77 | 183.51 | 0.4644 | -767.0 | -665.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -24.72 | 211.60 | -0.50 | 179.05 | 0.4785 | -800.0 | -606.8 | |
| 0.00 | 2.09 | 0.00 | 1.24 | -29.00 | 204.86 | -7.24 | 168.48 | 0.5536 | -689.0 | -598.5 | |
| 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. | |