SDO HMI 2014-06-06 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.43 | 0.00 | 10.03 | 4.67 | 259.17 | -28.62 | 78.03 | 0.4806 | -77.3 | 5.0 | |
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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 | 1.63 | 0.00 | 0.84 | 6.26 | 273.32 | -14.47 | 66.17 | 0.2727 | -877.0 | -618.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 5.83 | 273.21 | -14.58 | 67.80 | 0.2717 | -853.0 | -651.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 4.79 | 273.07 | -14.72 | 71.60 | 0.2679 | -647.0 | -530.2 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 3.17 | 272.91 | -14.88 | 77.67 | 0.2636 | -977.0 | -774.0 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 5.22 | 271.29 | -16.50 | 72.05 | 0.2987 | -908.0 | -669.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 2.96 | 270.31 | -17.48 | 80.09 | 0.3058 | -947.0 | -685.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 8.30 | 260.24 | -27.55 | 72.42 | 0.4820 | 600.0 | 443.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 7.93 | 259.99 | -27.80 | 73.29 | 0.4842 | 440.0 | 323.0 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 5.39 | 258.86 | -28.93 | 78.89 | 0.4928 | 771.0 | 588.2 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 5.89 | 255.23 | -32.56 | 79.09 | 0.5473 | 435.0 | 423.2 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 7.36 | 254.28 | -33.51 | 76.77 | 0.5646 | 702.0 | 598.8 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 6.08 | 249.06 | -38.73 | 80.29 | 0.6334 | 564.0 | 418.6 | |
| 0.00 | 1.00 | 0.00 | 0.65 | -1.33 | 246.92 | -40.87 | 91.98 | 0.6568 | -155.0 | -93.4 | |
| 0.00 | 1.00 | 0.00 | 0.68 | 1.39 | 243.99 | -43.80 | 87.95 | 0.6947 | 530.0 | 424.6 | |
| 0.00 | 1.63 | 0.00 | 1.13 | 2.46 | 243.19 | -44.60 | 86.46 | 0.7052 | 162.0 | 238.3 | |
| 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. | |