SDO HMI 2014-07-10 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 | 17.90 | 0.00 | 9.88 | -21.66 | 198.97 | -2.64 | 174.35 | 0.4413 | -65.8 | -21.9 | |
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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 | 1.00 | 0.00 | 0.55 | -22.36 | 206.04 | 4.43 | 189.21 | 0.4485 | 537.0 | 407.4 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -22.05 | 204.32 | 2.71 | 185.74 | 0.4401 | 768.0 | 655.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.73 | 203.86 | 2.25 | 185.28 | 0.4027 | 788.0 | 614.0 | |
| 0.00 | 3.09 | 0.00 | 1.70 | -22.05 | 203.63 | 2.02 | 184.28 | 0.4391 | 781.0 | 700.3 | |
| 0.00 | 1.82 | 0.00 | 1.00 | -21.88 | 203.36 | 1.75 | 183.75 | 0.4361 | 902.0 | 761.9 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -21.98 | 202.97 | 1.36 | 182.90 | 0.4374 | 740.0 | 567.0 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -27.04 | 199.87 | -1.74 | 176.98 | 0.5154 | -708.0 | -550.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.67 | 196.96 | -4.65 | 169.14 | 0.4071 | -886.0 | -741.0 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -20.59 | 194.05 | -7.56 | 163.37 | 0.4323 | -811.0 | -624.4 | |
| 0.00 | 2.09 | 0.00 | 1.15 | -20.55 | 193.79 | -7.82 | 162.81 | 0.4330 | -925.0 | -780.0 | |
| 0.00 | 1.73 | 0.00 | 0.95 | -20.76 | 193.64 | -7.96 | 162.67 | 0.4367 | -845.0 | -637.5 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -21.89 | 191.65 | -9.96 | 159.65 | 0.4633 | -603.0 | -518.0 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -22.26 | 191.59 | -10.02 | 159.84 | 0.4690 | -594.0 | -499.3 | |
| 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. | |