SDO HMI 2014-08-24 01:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.70 | 114.46 | 35.06 | 152.25 | -4.68 | 33.35 | 67.42 | 262.09 | 0.9303 | 353.8 | 273.5 | |
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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 |
| 1.62 | 84.62 | 2.32 | 115.59 | -4.35 | 34.98 | 69.05 | 262.73 | 0.9402 | 9.3 | 433.1 | |
| 0.00 | 1.35 | 0.00 | 1.93 | -5.76 | 34.71 | 68.77 | 261.20 | 0.9400 | 103.0 | 56.9 | |
| 0.00 | 3.23 | 0.00 | 4.61 | -5.32 | 34.60 | 68.66 | 261.64 | 0.9389 | 178.0 | 85.2 | |
| 0.45 | 1.53 | 0.63 | 2.15 | -5.05 | 34.36 | 68.43 | 261.89 | 0.9372 | 106.2 | 76.2 | |
| 22.10 | -1.00 | 30.39 | -1.00 | -4.72 | 33.96 | 68.03 | 262.16 | 0.9345 | 541.7 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.84 | -5.61 | 33.10 | 67.17 | 261.07 | 0.9301 | 298.0 | 387.1 | |
| 0.00 | 6.11 | 0.00 | 7.65 | -4.35 | 31.77 | 65.84 | 262.17 | 0.9200 | 273.0 | 170.0 | |
| 0.00 | 1.26 | 0.00 | 1.57 | -5.10 | 31.61 | 65.67 | 261.34 | 0.9198 | 459.0 | 338.5 | |
| 0.00 | 2.16 | 0.00 | 2.49 | -4.08 | 29.63 | 63.70 | 262.08 | 0.9046 | -254.0 | -176.5 | |
| 0.00 | 0.90 | 0.00 | 1.03 | -5.03 | 29.37 | 63.44 | 260.98 | 0.9040 | -126.0 | -36.4 | |
| 0.63 | 2.69 | 0.71 | 3.06 | -4.24 | 29.18 | 63.24 | 261.81 | 0.9015 | -490.7 | -432.3 | |
| 0.90 | 7.46 | 1.01 | 8.47 | -3.92 | 29.06 | 63.13 | 262.14 | 0.9002 | -640.7 | -538.0 | |
| 0.00 | 1.89 | 0.00 | 2.14 | -5.55 | 28.99 | 63.06 | 260.34 | 0.9018 | -470.0 | -407.3 | |
| 0.00 | 0.63 | 0.00 | 0.72 | -6.04 | 28.95 | 63.02 | 259.80 | 0.9022 | -426.0 | -356.7 | |
| 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. | |