SDO HMI 2014-08-24 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.06 | 102.30 | 29.71 | 154.63 | -4.64 | 33.38 | 70.19 | 262.61 | 0.9466 | 261.5 | 260.7 | |
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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 |
| 1.08 | 3.68 | 1.78 | 6.10 | -4.35 | 34.96 | 71.77 | 263.17 | 0.9551 | -70.6 | -185.0 | |
| 0.00 | 1.98 | 0.00 | 3.26 | -4.95 | 34.81 | 71.62 | 262.53 | 0.9549 | -396.0 | -277.8 | |
| 4.94 | 74.33 | 7.94 | 115.74 | -4.63 | 34.44 | 71.25 | 262.80 | 0.9527 | 329.7 | 457.0 | |
| 2.34 | -3.00 | 3.74 | -3.00 | -4.41 | 34.39 | 71.20 | 263.02 | 0.9522 | 506.2 | 999999 | |
| 0.00 | 1.71 | 0.00 | 2.79 | -5.36 | 34.63 | 71.44 | 262.07 | 0.9543 | 88.0 | 65.9 | |
| 8.81 | -3.00 | 13.66 | -3.00 | -4.91 | 33.66 | 70.47 | 262.38 | 0.9488 | 626.7 | 999999 | |
| 0.00 | 1.62 | 0.00 | 2.31 | -4.51 | 32.06 | 68.87 | 262.53 | 0.9393 | 550.0 | 338.5 | |
| 1.89 | 3.24 | 2.59 | 4.44 | -4.35 | 31.19 | 68.00 | 262.56 | 0.9339 | -75.3 | -27.2 | |
| 0.00 | 1.26 | 0.00 | 1.69 | -4.06 | 30.81 | 67.62 | 262.80 | 0.9313 | -380.0 | -286.4 | |
| 0.00 | 0.99 | 0.00 | 1.31 | -3.75 | 30.52 | 67.33 | 263.08 | 0.9291 | -339.0 | -286.0 | |
| 0.00 | 1.17 | 0.00 | 1.50 | -3.99 | 29.69 | 66.50 | 262.68 | 0.9240 | -281.0 | -227.8 | |
| 0.00 | 8.45 | 0.00 | 10.62 | -3.81 | 29.21 | 66.02 | 262.78 | 0.9206 | -643.0 | -500.2 | |
| 0.00 | 1.80 | 0.00 | 2.26 | -4.24 | 29.20 | 66.01 | 262.32 | 0.9210 | -416.0 | -358.2 | |
| 0.00 | 1.17 | 0.00 | 1.48 | -4.83 | 29.23 | 66.04 | 261.69 | 0.9219 | -348.0 | -226.7 | |
| 0.00 | 0.90 | 0.00 | 1.13 | -5.58 | 29.00 | 65.81 | 260.85 | 0.9213 | -203.0 | -254.0 | |
| 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. | |