SDO HMI 2014-06-06 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.75 | 0.00 | 10.22 | 4.30 | 263.76 | -22.38 | 77.51 | 0.3856 | -89.9 | -130.7 | |
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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 | 2.35 | 0.00 | 1.20 | 5.22 | 273.40 | -12.75 | 67.38 | 0.2391 | -912.0 | -719.5 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 4.40 | 273.04 | -13.11 | 71.15 | 0.2400 | -890.0 | -691.4 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 3.85 | 272.58 | -13.57 | 73.88 | 0.2447 | -789.0 | -477.0 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 3.73 | 272.36 | -13.79 | 74.59 | 0.2478 | -836.0 | -503.4 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 3.61 | 271.67 | -14.48 | 75.73 | 0.2586 | -754.0 | -629.8 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 5.17 | 271.29 | -14.85 | 70.48 | 0.2721 | -921.0 | -705.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 2.36 | 270.11 | -16.04 | 81.41 | 0.2804 | -901.0 | -782.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -2.53 | 268.80 | -17.35 | 98.35 | 0.3025 | -724.0 | -525.1 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 5.83 | 256.24 | -29.90 | 78.38 | 0.5084 | 782.0 | 659.4 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 6.14 | 255.26 | -30.88 | 78.12 | 0.5236 | 603.0 | 503.3 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 5.89 | 255.28 | -30.87 | 78.58 | 0.5227 | 694.0 | 533.6 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 4.64 | 253.88 | -32.27 | 81.31 | 0.5404 | 678.0 | 541.2 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 8.01 | 252.28 | -33.87 | 75.78 | 0.5714 | 775.0 | 576.8 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -0.84 | 250.98 | -35.17 | 91.41 | 0.5783 | 426.0 | 451.0 | |
| 0.00 | 0.63 | 0.00 | 0.39 | 8.79 | 249.87 | -36.28 | 75.32 | 0.6067 | 648.0 | 573.7 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 4.37 | 249.86 | -36.29 | 82.60 | 0.5973 | 682.0 | 515.9 | |
| 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. | |