SDO HMI 2014-09-20 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.58 | 273.70 | 67.33 | 319.06 | -9.56 | 263.78 | -62.83 | 104.11 | 0.9044 | 134.9 | 72.9 | |
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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 |
| 0.00 | 1.60 | 0.00 | 1.59 | -8.14 | 268.24 | -58.36 | 103.66 | 0.8693 | 492.0 | 415.6 | |
| 21.55 | 157.78 | 22.25 | 164.03 | -8.30 | 267.08 | -59.53 | 103.54 | 0.8792 | 951.3 | 236.0 | |
| 9.58 | -2.00 | 10.08 | -2.00 | -8.43 | 266.49 | -60.11 | 103.53 | 0.8841 | 515.4 | 999999 | |
| 0.00 | 1.69 | 0.00 | 1.85 | -9.00 | 265.26 | -61.34 | 103.86 | 0.8945 | -256.0 | -203.4 | |
| 0.00 | 2.66 | 0.00 | 2.90 | -8.39 | 265.37 | -61.23 | 103.22 | 0.8927 | 246.0 | 189.3 | |
| 0.00 | 2.22 | 0.00 | 2.43 | -8.65 | 265.30 | -61.31 | 103.49 | 0.8937 | 210.0 | 76.9 | |
| 1.06 | 7.63 | 1.15 | 8.31 | -7.83 | 265.46 | -61.15 | 102.62 | 0.8911 | 365.1 | 325.1 | |
| 0.00 | 2.39 | 0.00 | 2.66 | -7.91 | 264.73 | -61.88 | 102.54 | 0.8967 | 146.0 | 60.5 | |
| 0.00 | 1.06 | 0.00 | 1.25 | -7.96 | 263.18 | -63.43 | 102.24 | 0.9081 | -391.0 | -367.5 | |
| 0.00 | 0.80 | 0.00 | 0.99 | -9.02 | 262.00 | -64.60 | 103.12 | 0.9178 | -217.0 | -263.8 | |
| 0.00 | 1.33 | 0.00 | 1.64 | -8.63 | 261.92 | -64.69 | 102.68 | 0.9178 | -538.0 | -450.8 | |
| 17.38 | 94.54 | 24.19 | 131.41 | -11.57 | 259.67 | -66.94 | 105.30 | 0.9360 | -559.0 | -151.4 | |
| 7.01 | -12.00 | 9.66 | -12.00 | -10.72 | 259.67 | -66.93 | 104.41 | 0.9349 | -288.9 | 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. | |