SDO HMI 2014-08-07 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.45 | 52.35 | 22.70 | 68.79 | -20.54 | 251.32 | 63.42 | 244.79 | 0.9269 | 98.2 | -39.4 | |
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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 | 1.99 | 0.00 | 2.75 | -19.85 | 252.96 | 65.06 | 245.96 | 0.9354 | -218.0 | -208.2 | |
| 0.00 | 1.54 | 0.00 | 2.13 | -20.02 | 252.93 | 65.03 | 245.78 | 0.9355 | -280.0 | -233.0 | |
| 2.71 | 27.67 | 3.68 | 38.07 | -19.89 | 252.38 | 64.47 | 245.76 | 0.9321 | 509.9 | 13.6 | |
| 1.63 | -3.00 | 2.22 | -3.00 | -20.30 | 252.46 | 64.56 | 245.36 | 0.9333 | 582.4 | 999999 | |
| 0.00 | 1.08 | 0.00 | 1.44 | -19.68 | 251.91 | 64.01 | 245.86 | 0.9291 | 427.0 | 429.8 | |
| 5.79 | -3.00 | 7.95 | -3.00 | -20.64 | 252.50 | 64.60 | 245.02 | 0.9341 | 357.1 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.92 | -19.70 | 250.76 | 62.86 | 245.52 | 0.9222 | 444.0 | 411.4 | |
| 0.00 | 3.44 | 0.00 | 4.30 | -20.50 | 250.12 | 62.22 | 244.50 | 0.9198 | -291.0 | -39.9 | |
| 4.61 | 8.32 | 5.60 | 10.10 | -20.81 | 249.23 | 61.33 | 243.91 | 0.9149 | -39.5 | 75.3 | |
| 0.00 | 0.72 | 0.00 | 0.87 | -21.11 | 248.90 | 61.00 | 243.49 | 0.9135 | -355.0 | -308.8 | |
| 0.90 | 2.08 | 1.09 | 2.50 | -21.23 | 248.71 | 60.81 | 243.31 | 0.9125 | -342.9 | -254.2 | |
| 1.81 | 2.98 | 2.16 | 3.56 | -21.44 | 248.45 | 60.55 | 243.01 | 0.9113 | -510.4 | -453.8 | |
| 0.00 | 0.54 | 0.00 | 0.64 | -21.58 | 248.22 | 60.32 | 242.79 | 0.9102 | -555.0 | -507.5 | |
| 0.00 | 1.27 | 0.00 | 1.51 | -21.95 | 248.21 | 60.31 | 242.40 | 0.9110 | -469.0 | -432.1 | |
| 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. | |