SDO HMI 2014-07-09 19:13:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.52 | 0.00 | 7.55 | -22.57 | 198.40 | -5.87 | 168.65 | 0.4598 | -66.5 | -87.2 | |
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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 | 0.45 | -22.04 | 204.01 | -0.25 | 179.47 | 0.4372 | 867.0 | 679.8 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.34 | 203.75 | -0.52 | 178.92 | 0.4421 | 544.0 | 468.9 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -22.20 | 203.71 | -0.55 | 178.84 | 0.4400 | 681.0 | 554.7 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -21.56 | 203.32 | -0.94 | 177.96 | 0.4300 | 905.0 | 688.5 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -26.93 | 200.13 | -4.13 | 172.82 | 0.5165 | -781.0 | -545.4 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.59 | 199.61 | -4.65 | 170.43 | 0.4520 | 711.0 | 510.6 | |
| 0.00 | 2.45 | 0.00 | 1.33 | -19.77 | 197.26 | -7.00 | 163.97 | 0.4170 | -846.0 | -577.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -21.22 | 196.17 | -8.09 | 162.73 | 0.4437 | -773.0 | -573.4 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -20.60 | 194.06 | -10.20 | 158.08 | 0.4457 | -753.0 | -641.4 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -22.05 | 191.81 | -12.45 | 155.29 | 0.4799 | -708.0 | -607.7 | |
| 0.00 | 0.73 | 0.00 | 0.48 | -32.43 | 183.28 | -20.99 | 152.75 | 0.6626 | -579.0 | -507.8 | |
| 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. | |