SDO HMI 2014-06-07 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 |
| 0.00 | 21.55 | 0.00 | 11.33 | 5.07 | 258.60 | -15.96 | 62.67 | 0.2977 | 203.3 | 164.7 | |
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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 | 0.72 | 5.32 | 273.83 | -0.73 | 7.88 | 0.0926 | -1125.0 | -865.1 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 4.92 | 273.83 | -0.73 | 8.52 | 0.0858 | -686.0 | -531.0 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 5.29 | 271.14 | -3.42 | 33.15 | 0.1090 | -790.0 | -520.7 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 1.94 | 269.22 | -5.33 | 70.71 | 0.0988 | -1022.0 | -852.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 2.79 | 269.19 | -5.36 | 63.11 | 0.1052 | -886.0 | -693.4 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 5.58 | 259.85 | -14.70 | 69.22 | 0.2714 | 842.0 | 605.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 5.92 | 258.92 | -15.63 | 69.21 | 0.2879 | 790.0 | 555.6 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 6.74 | 256.37 | -18.19 | 69.46 | 0.3324 | 710.0 | 569.1 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 9.88 | 256.12 | -18.43 | 61.33 | 0.3565 | 705.0 | 520.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 9.66 | 256.04 | -18.52 | 61.98 | 0.3562 | 816.0 | 673.4 | |
| 0.00 | 2.63 | 0.00 | 1.43 | 9.36 | 252.13 | -22.42 | 66.79 | 0.4112 | 806.0 | 520.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 5.49 | 250.31 | -24.25 | 76.98 | 0.4213 | 688.0 | 531.9 | |
| 0.00 | 1.45 | 0.00 | 0.79 | -0.51 | 249.65 | -24.91 | 91.37 | 0.4230 | 772.0 | 592.3 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 9.12 | 249.22 | -25.34 | 69.60 | 0.4527 | 623.0 | 541.8 | |
| 0.00 | 2.44 | 0.00 | 1.37 | -0.20 | 246.34 | -28.21 | 90.57 | 0.4747 | 806.0 | 633.3 | |
| 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. | |