SDO HMI 2014-07-07 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.36 | 24.25 | 2.93 | 16.02 | 12.15 | 277.83 | 40.90 | 284.50 | 0.6633 | -307.7 | -138.5 | |
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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 | 0.64 | 0.00 | 0.44 | 10.76 | 281.53 | 44.60 | 281.72 | 0.7068 | -424.0 | -319.6 | |
| 0.00 | 0.45 | 0.00 | 0.32 | 11.13 | 281.47 | 44.55 | 282.26 | 0.7066 | -398.0 | -375.0 | |
| 0.00 | 1.18 | 0.00 | 0.79 | 9.09 | 279.40 | 42.48 | 279.60 | 0.6786 | -661.0 | -530.3 | |
| 0.00 | 2.63 | 0.00 | 1.78 | 10.81 | 279.60 | 42.68 | 282.09 | 0.6832 | -767.0 | -459.0 | |
| 4.36 | 6.36 | 2.93 | 4.27 | 11.33 | 278.98 | 42.05 | 282.96 | 0.6762 | -743.2 | -516.9 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 11.39 | 278.19 | 41.27 | 283.20 | 0.6665 | -750.0 | -666.6 | |
| 0.00 | 0.82 | 0.00 | 0.54 | 12.88 | 278.27 | 41.35 | 285.39 | 0.6702 | -398.0 | -278.1 | |
| 0.00 | 2.36 | 0.00 | 1.58 | 13.37 | 278.33 | 41.41 | 286.10 | 0.6720 | -642.0 | -466.3 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 12.39 | 278.13 | 41.21 | 284.69 | 0.6675 | -581.0 | -476.0 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 12.54 | 278.08 | 41.16 | 284.94 | 0.6671 | -451.0 | -447.0 | |
| 0.00 | 0.36 | 0.00 | 0.24 | 13.10 | 278.15 | 41.23 | 285.75 | 0.6692 | -588.0 | -600.8 | |
| 0.00 | 1.91 | 0.00 | 1.22 | 12.98 | 275.63 | 38.70 | 286.22 | 0.6368 | 726.0 | 537.0 | |
| 0.00 | 1.64 | 0.00 | 1.05 | 13.99 | 275.22 | 38.30 | 287.91 | 0.6342 | 732.0 | 574.8 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 13.88 | 274.80 | 37.88 | 287.87 | 0.6285 | 515.0 | 436.7 | |
| 0.00 | 2.18 | 0.00 | 1.36 | 14.12 | 273.50 | 36.58 | 288.68 | 0.6122 | 656.0 | 517.4 | |
| 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. | |