SDO HMI 2014-07-03 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.62 | 0.00 | 9.89 | 6.43 | 261.68 | -26.54 | 80.88 | 0.4535 | 515.5 | 504.0 | |
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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 | 0.91 | 0.00 | 0.46 | 7.46 | 279.62 | -8.60 | 62.75 | 0.1676 | -695.0 | -563.7 | |
| 0.00 | 0.64 | 0.00 | 0.32 | 1.64 | 279.49 | -8.72 | 99.43 | 0.1544 | -803.0 | -653.3 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 11.06 | 267.93 | -20.29 | 67.42 | 0.3701 | 836.0 | 733.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 10.72 | 267.42 | -20.79 | 68.74 | 0.3759 | 973.0 | 753.6 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 8.38 | 267.37 | -20.85 | 74.86 | 0.3663 | 751.0 | 576.7 | |
| 0.00 | 1.82 | 0.00 | 1.01 | 8.87 | 261.36 | -26.85 | 76.63 | 0.4606 | 794.0 | 563.2 | |
| 0.00 | 1.64 | 0.00 | 0.92 | 8.52 | 260.84 | -27.38 | 77.58 | 0.4676 | 844.0 | 797.7 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -1.18 | 258.54 | -29.68 | 97.81 | 0.5016 | 832.0 | 642.5 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 7.45 | 258.25 | -29.97 | 80.52 | 0.5042 | 772.0 | 683.9 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -4.04 | 258.32 | -29.90 | 103.28 | 0.5129 | 470.0 | 463.5 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 7.38 | 257.93 | -30.29 | 80.73 | 0.5088 | 559.0 | 393.9 | |
| 0.00 | 2.63 | 0.00 | 1.52 | 7.68 | 257.70 | -30.52 | 80.20 | 0.5128 | 706.0 | 536.4 | |
| 0.00 | 1.00 | 0.00 | 0.62 | 5.46 | 250.74 | -37.48 | 85.09 | 0.6102 | 662.0 | 495.6 | |
| 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. | |