SDO HMI 2014-09-09 08:08:51 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.08 | 208.18 | 34.02 | 164.95 | -16.28 | 64.64 | -46.03 | 117.73 | 0.7815 | 200.6 | 48.7 | |
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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 |
| 6.33 | 134.96 | 4.80 | 102.67 | -16.13 | 66.96 | -43.71 | 118.68 | 0.7590 | 1100.4 | 261.5 | |
| 3.66 | -1.00 | 2.78 | -1.00 | -16.33 | 66.86 | -43.81 | 118.87 | 0.7609 | 827.2 | 999999 | |
| 17.75 | -1.00 | 13.53 | -1.00 | -16.03 | 66.59 | -44.08 | 118.37 | 0.7621 | 894.2 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.78 | -16.73 | 64.68 | -45.99 | 118.22 | 0.7838 | 221.0 | 227.7 | |
| 1.16 | 6.24 | 0.92 | 4.94 | -16.10 | 64.47 | -46.20 | 117.37 | 0.7831 | 487.2 | 429.5 | |
| 5.53 | 8.03 | 4.50 | 6.53 | -16.00 | 63.16 | -47.51 | 116.62 | 0.7951 | -758.2 | -530.9 | |
| 0.00 | 0.98 | 0.00 | 0.81 | -16.84 | 62.84 | -47.83 | 117.45 | 0.8016 | -518.0 | -458.9 | |
| 0.45 | 2.94 | 0.37 | 2.44 | -16.91 | 62.53 | -48.14 | 117.38 | 0.8047 | -684.6 | -545.5 | |
| 0.00 | 1.78 | 0.00 | 1.49 | -16.43 | 62.07 | -48.59 | 116.62 | 0.8069 | -616.0 | -567.1 | |
| 0.00 | 1.16 | 0.00 | 0.98 | -16.58 | 61.54 | -49.13 | 116.55 | 0.8124 | -551.0 | -509.1 | |
| 0.00 | 3.03 | 0.00 | 2.59 | -16.85 | 61.10 | -49.56 | 116.67 | 0.8174 | -691.0 | -564.4 | |
| 0.00 | 1.07 | 0.00 | 0.94 | -17.76 | 60.52 | -50.15 | 117.44 | 0.8260 | -574.0 | -528.8 | |
| 2.85 | 45.76 | 2.45 | 39.68 | -16.46 | 60.75 | -49.92 | 116.07 | 0.8190 | -823.7 | -324.8 | |
| 0.00 | 1.25 | 0.00 | 1.10 | -17.52 | 59.96 | -50.71 | 116.93 | 0.8299 | -422.0 | -359.5 | |
| 5.35 | -13.00 | 4.67 | -13.00 | -16.75 | 60.15 | -50.52 | 116.14 | 0.8254 | -466.9 | 999999 | |
| 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. | |