SDO HMI 2014-07-09 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 |
| 0.00 | 16.08 | 0.00 | 9.22 | -22.49 | 199.56 | -14.73 | 152.27 | 0.5047 | 52.2 | 31.0 | |
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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 | 1.09 | 0.00 | 0.60 | -20.98 | 206.64 | -7.65 | 163.41 | 0.4372 | 790.0 | 571.3 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -21.74 | 204.81 | -9.48 | 160.36 | 0.4573 | 764.0 | 593.4 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -21.62 | 203.18 | -11.11 | 157.23 | 0.4648 | 1073.0 | 904.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -21.83 | 203.00 | -11.29 | 157.08 | 0.4687 | 723.0 | 630.2 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -21.66 | 202.81 | -11.48 | 156.59 | 0.4675 | 847.0 | 643.4 | |
| 0.00 | 1.82 | 0.00 | 1.08 | -27.09 | 200.32 | -13.97 | 157.16 | 0.5559 | -871.0 | -717.0 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -26.57 | 199.51 | -14.78 | 155.57 | 0.5539 | -760.0 | -581.3 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -23.21 | 199.03 | -15.26 | 151.77 | 0.5136 | 612.0 | 434.8 | |
| 0.00 | 0.82 | 0.00 | 0.47 | -22.70 | 198.81 | -15.48 | 150.92 | 0.5086 | 521.0 | 496.9 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -19.15 | 197.01 | -17.29 | 143.96 | 0.4790 | -772.0 | -593.4 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -20.16 | 195.94 | -18.36 | 143.65 | 0.5007 | -817.0 | -626.8 | |
| 0.00 | 1.82 | 0.00 | 1.08 | -22.45 | 192.75 | -21.54 | 142.16 | 0.5553 | -813.0 | -642.9 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -18.72 | 189.78 | -24.52 | 133.74 | 0.5461 | -618.0 | -412.2 | |
| 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. | |