SDO HMI 2014-06-07 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.19 | 0.00 | 10.52 | 4.51 | 263.52 | -13.77 | 61.41 | 0.2568 | 14.6 | -148.9 | |
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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 |
| 0.00 | 3.62 | 0.00 | 1.80 | 5.31 | 273.73 | -3.57 | 34.01 | 0.1113 | -963.0 | -798.2 | |
| 0.00 | 2.81 | 0.00 | 1.40 | 5.13 | 273.27 | -4.03 | 38.27 | 0.1134 | -644.0 | -623.9 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 4.30 | 273.00 | -4.30 | 45.15 | 0.1059 | -1039.0 | -770.8 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 3.39 | 271.81 | -5.49 | 58.53 | 0.1124 | -820.0 | -627.6 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.21 | 271.63 | -5.67 | 60.75 | 0.1136 | -776.0 | -626.6 | |
| 0.00 | 1.90 | 0.00 | 0.95 | 1.51 | 269.03 | -8.27 | 79.91 | 0.1467 | -672.0 | -497.7 | |
| 0.00 | 1.99 | 0.00 | 1.06 | 5.70 | 256.39 | -20.90 | 74.48 | 0.3701 | 761.0 | 568.0 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 1.40 | 254.65 | -22.64 | 86.47 | 0.3873 | 799.0 | 590.4 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -0.52 | 254.33 | -22.97 | 91.42 | 0.3920 | 801.0 | 536.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 8.74 | 249.44 | -27.86 | 71.86 | 0.4879 | 713.0 | 551.6 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 10.25 | 248.68 | -28.62 | 69.38 | 0.5056 | 670.0 | 543.8 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -0.18 | 246.33 | -30.97 | 90.41 | 0.5167 | 730.0 | 627.2 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 5.49 | 244.99 | -32.31 | 79.86 | 0.5426 | 630.0 | 533.7 | |
| 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. | |