SDO HMI 2014-10-30 15:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.54 | 57.62 | 16.75 | 53.05 | -15.90 | 99.75 | -54.22 | 112.16 | 0.8442 | 374.0 | 157.9 | |
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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 |
| 10.31 | 24.26 | 9.21 | 21.70 | -15.81 | 100.90 | -53.07 | 112.42 | 0.8342 | 694.5 | 380.5 | |
| 0.00 | 1.73 | 0.00 | 1.57 | -15.29 | 100.21 | -53.76 | 111.60 | 0.8389 | 384.0 | 250.1 | |
| 7.54 | 16.81 | 6.89 | 15.42 | -15.88 | 99.93 | -54.04 | 112.18 | 0.8429 | 596.4 | 346.7 | |
| 0.00 | 1.73 | 0.00 | 1.58 | -15.19 | 99.82 | -54.14 | 111.36 | 0.8420 | 76.0 | 42.1 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -16.31 | 99.11 | -54.86 | 112.41 | 0.8510 | 151.0 | 105.3 | |
| 0.69 | 2.60 | 0.65 | 2.42 | -15.96 | 99.20 | -54.76 | 112.04 | 0.8493 | 101.0 | 35.3 | |
| 0.00 | 0.78 | 0.00 | 0.74 | -16.14 | 98.80 | -55.17 | 112.12 | 0.8532 | 183.0 | 138.9 | |
| 0.00 | 1.65 | 0.00 | 1.54 | -15.59 | 98.97 | -55.00 | 111.56 | 0.8504 | -505.0 | -376.9 | |
| 0.00 | 0.95 | 0.00 | 0.92 | -16.21 | 97.83 | -56.14 | 111.90 | 0.8614 | 359.0 | 329.7 | |
| 0.00 | 2.17 | 0.00 | 2.08 | -15.41 | 98.00 | -55.96 | 111.05 | 0.8581 | -219.0 | -284.6 | |
| 0.00 | 1.73 | 0.00 | 1.70 | -15.53 | 97.11 | -56.86 | 110.93 | 0.8658 | -313.0 | -311.0 | |
| 0.00 | 1.39 | 0.00 | 1.52 | -18.99 | 94.39 | -59.57 | 113.96 | 0.8941 | -140.0 | -239.2 | |
| 0.00 | 1.56 | 0.00 | 1.62 | -16.59 | 95.45 | -58.51 | 111.64 | 0.8812 | -543.0 | -534.7 | |
| 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. | |