SDO HMI 2014-07-10 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.26 | 0.00 | 9.09 | -23.02 | 199.09 | -0.86 | 179.34 | 0.4632 | 132.8 | 90.1 | |
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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 | 1.54 | 0.00 | 0.86 | -22.46 | 206.02 | 6.06 | 192.43 | 0.4551 | 380.0 | 224.5 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.07 | 204.38 | 4.43 | 189.30 | 0.4443 | 653.0 | 474.4 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -22.18 | 204.25 | 4.30 | 188.99 | 0.4456 | 659.0 | 543.6 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -22.07 | 203.92 | 3.96 | 188.34 | 0.4432 | 916.0 | 695.2 | |
| 0.00 | 1.91 | 0.00 | 1.05 | -22.17 | 203.73 | 3.77 | 187.91 | 0.4443 | 753.0 | 630.2 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.87 | 203.42 | 3.46 | 187.37 | 0.4389 | 882.0 | 784.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.10 | 203.39 | 3.44 | 187.24 | 0.4425 | 670.0 | 559.5 | |
| 0.00 | 0.64 | 0.00 | 0.35 | -22.50 | 198.52 | -1.44 | 177.01 | 0.4459 | 588.0 | 469.6 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -22.09 | 196.51 | -3.44 | 172.74 | 0.4424 | -816.0 | -719.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -22.03 | 196.29 | -3.67 | 172.25 | 0.4418 | -822.0 | -570.7 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -20.76 | 193.70 | -6.26 | 166.23 | 0.4298 | -758.0 | -630.0 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.42 | 193.52 | -6.44 | 165.64 | 0.4254 | -686.0 | -610.4 | |
| 0.00 | 1.82 | 0.00 | 1.13 | -30.70 | 184.75 | -15.21 | 158.23 | 0.6104 | -692.0 | -518.0 | |
| 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. | |