SDO HMI 2014-09-22 21:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.93 | 25.48 | 6.34 | 18.70 | -15.05 | 249.55 | -42.41 | 118.01 | 0.7391 | 140.7 | -116.2 | |
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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 | 0.97 | 0.00 | 0.68 | -15.73 | 253.37 | -38.59 | 121.04 | 0.7031 | 490.0 | 327.3 | |
| 5.57 | 13.98 | 3.95 | 9.93 | -15.28 | 251.73 | -40.23 | 119.46 | 0.7178 | 927.2 | 490.9 | |
| 3.36 | -2.00 | 2.39 | -2.00 | -15.48 | 251.60 | -40.36 | 119.63 | 0.7203 | 661.1 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.81 | -13.72 | 251.55 | -40.41 | 117.37 | 0.7115 | 612.0 | 522.2 | |
| 0.00 | 1.15 | 0.00 | 0.88 | -14.09 | 246.84 | -45.12 | 115.35 | 0.7628 | -635.0 | -573.2 | |
| 0.00 | 0.97 | 0.00 | 0.74 | -13.95 | 246.65 | -45.30 | 115.09 | 0.7640 | -728.0 | -616.7 | |
| 0.00 | 1.24 | 0.00 | 0.96 | -15.17 | 246.28 | -45.68 | 116.38 | 0.7730 | -656.0 | -563.4 | |
| 0.00 | 0.80 | 0.00 | 0.62 | -15.25 | 246.13 | -45.83 | 116.40 | 0.7749 | -426.0 | -461.8 | |
| 0.00 | 1.95 | 0.00 | 1.53 | -15.36 | 245.64 | -46.31 | 116.29 | 0.7801 | -425.0 | -357.6 | |
| 0.00 | 2.21 | 0.00 | 1.73 | -14.71 | 245.69 | -46.27 | 115.54 | 0.7769 | -714.0 | -628.4 | |
| 0.00 | 1.06 | 0.00 | 0.82 | -14.02 | 245.88 | -46.08 | 114.80 | 0.7721 | -602.0 | -496.2 | |
| 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. | |