SDO HMI 2014-07-07 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.73 | 26.25 | 2.48 | 17.19 | 12.36 | 277.71 | 40.24 | 284.94 | 0.6552 | -109.0 | -126.3 | |
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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 | 1.45 | 0.00 | 1.00 | 11.97 | 281.18 | 43.71 | 283.59 | 0.6978 | -276.0 | -280.7 | |
| 0.00 | 1.73 | 0.00 | 1.16 | 10.77 | 279.63 | 42.16 | 282.12 | 0.6767 | -759.0 | -442.8 | |
| 3.73 | 5.63 | 2.48 | 3.75 | 11.29 | 279.01 | 41.54 | 283.00 | 0.6697 | -751.4 | -540.1 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 11.38 | 278.20 | 40.73 | 283.30 | 0.6596 | -761.0 | -668.2 | |
| 0.00 | 1.54 | 0.00 | 1.02 | 13.33 | 278.37 | 40.90 | 286.17 | 0.6656 | -564.0 | -516.3 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 12.41 | 278.14 | 40.67 | 284.85 | 0.6608 | -608.0 | -510.0 | |
| 0.00 | 3.09 | 0.00 | 2.03 | 12.60 | 277.93 | 40.46 | 285.19 | 0.6585 | -612.0 | -387.9 | |
| 0.00 | 2.54 | 0.00 | 1.66 | 12.03 | 277.46 | 39.99 | 284.44 | 0.6513 | -619.0 | -441.9 | |
| 0.00 | 0.82 | 0.00 | 0.52 | 12.05 | 276.25 | 38.78 | 284.75 | 0.6356 | 461.0 | 362.9 | |
| 0.00 | 0.82 | 0.00 | 0.52 | 12.58 | 275.98 | 38.51 | 285.66 | 0.6334 | 431.0 | 410.0 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 13.00 | 275.66 | 38.19 | 286.40 | 0.6302 | 762.0 | 600.6 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 14.16 | 275.40 | 37.93 | 288.29 | 0.6300 | 596.0 | 490.7 | |
| 0.00 | 1.64 | 0.00 | 1.04 | 13.98 | 275.24 | 37.77 | 288.06 | 0.6274 | 723.0 | 633.9 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 14.43 | 274.74 | 37.27 | 288.94 | 0.6222 | 632.0 | 562.0 | |
| 0.00 | 0.91 | 0.00 | 0.56 | 14.08 | 273.49 | 36.02 | 288.81 | 0.6048 | 662.0 | 574.5 | |
| 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. | |