SDO HMI 2014-06-30 01:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.67 | 293.25 | 100.05 | 627.67 | -20.33 | 258.97 | -74.44 | 111.70 | 0.9728 | 10.6 | -110.9 | |
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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 |
| 5.54 | 18.71 | 9.02 | 30.45 | -21.16 | 263.60 | -69.81 | 113.24 | 0.9539 | 516.1 | 304.6 | |
| 0.91 | 112.06 | 1.57 | 216.06 | -21.40 | 262.53 | -70.88 | 113.32 | 0.9591 | 178.6 | -365.8 | |
| 3.90 | -2.00 | 6.84 | -2.00 | -21.22 | 262.24 | -71.17 | 113.08 | 0.9603 | 134.0 | 999999 | |
| 0.00 | 3.09 | 0.00 | 6.22 | -22.61 | 260.13 | -73.28 | 114.17 | 0.9701 | -356.0 | -308.5 | |
| 0.00 | 0.91 | 0.00 | 1.83 | -22.38 | 260.10 | -73.31 | 113.93 | 0.9701 | -520.0 | -456.0 | |
| 4.81 | -2.00 | 9.20 | -2.00 | -21.75 | 260.84 | -72.57 | 113.40 | 0.9667 | -611.4 | 999999 | |
| 3.09 | 6.45 | 6.48 | 13.54 | -22.28 | 259.41 | -74.00 | 113.73 | 0.9726 | -307.4 | -230.1 | |
| 4.54 | -2.00 | 9.11 | -2.00 | -21.59 | 260.03 | -73.38 | 113.11 | 0.9698 | -501.7 | 999999 | |
| 0.00 | 3.00 | 0.00 | 7.07 | -22.79 | 257.86 | -75.55 | 114.02 | 0.9784 | -30.0 | -33.7 | |
| 0.00 | 1.82 | 0.00 | 3.30 | -20.20 | 261.42 | -71.99 | 111.90 | 0.9631 | 77.0 | -42.5 | |
| 1.54 | -2.00 | 3.52 | -2.00 | -22.17 | 258.19 | -75.22 | 113.44 | 0.9769 | -274.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 3.13 | -20.98 | 256.96 | -76.45 | 112.07 | 0.9804 | -188.0 | -155.4 | |
| 23.34 | 145.94 | 54.31 | 346.07 | -19.28 | 257.47 | -75.94 | 110.41 | 0.9780 | 173.7 | 28.0 | |
| 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. | |