SDO HMI 2014-07-29 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.51 | 0.00 | 10.91 | 12.22 | 259.69 | -45.04 | 77.98 | 0.7069 | 200.2 | 117.3 | |
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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 | 1.18 | 0.00 | 0.72 | 16.24 | 269.44 | -35.30 | 69.97 | 0.5926 | -690.0 | -569.0 | |
| 0.00 | 1.09 | 0.00 | 0.68 | 14.48 | 267.99 | -36.75 | 73.32 | 0.6069 | -682.0 | -564.8 | |
| 0.00 | 2.99 | 0.00 | 1.88 | 12.32 | 266.92 | -37.82 | 77.08 | 0.6168 | -582.0 | -454.0 | |
| 0.00 | 1.27 | 0.00 | 0.91 | 16.50 | 258.79 | -45.94 | 72.45 | 0.7250 | 248.0 | 225.5 | |
| 0.00 | 0.63 | 0.00 | 0.46 | 16.19 | 258.01 | -46.73 | 73.01 | 0.7334 | 511.0 | 389.4 | |
| 0.00 | 0.91 | 0.00 | 0.63 | 6.12 | 259.47 | -45.26 | 86.91 | 0.7096 | 587.0 | 529.0 | |
| 0.00 | 1.00 | 0.00 | 0.74 | 15.57 | 256.60 | -48.13 | 74.08 | 0.7483 | 441.0 | 311.5 | |
| 0.00 | 1.09 | 0.00 | 0.79 | 9.96 | 257.48 | -47.25 | 81.56 | 0.7335 | 554.0 | 452.0 | |
| 0.00 | 1.09 | 0.00 | 0.80 | 9.77 | 256.92 | -47.81 | 81.84 | 0.7400 | 660.0 | 551.2 | |
| 0.00 | 1.18 | 0.00 | 0.87 | 9.60 | 256.67 | -48.06 | 82.08 | 0.7428 | 620.0 | 471.3 | |
| 0.00 | 1.81 | 0.00 | 1.40 | 10.63 | 254.32 | -50.41 | 80.79 | 0.7696 | 314.0 | 248.4 | |
| 0.00 | 1.27 | 0.00 | 1.03 | 11.56 | 251.83 | -52.91 | 79.70 | 0.7965 | 422.0 | 407.6 | |
| 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. | |