SDO HMI 2014-11-26 05:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.13 | 276.44 | 111.97 | 711.96 | -16.13 | 241.02 | 77.54 | 253.20 | 0.9807 | -328.1 | -57.3 | |
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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 | 1.03 | 0.00 | 2.72 | -11.93 | 242.16 | 78.67 | 257.56 | 0.9833 | 49.0 | 73.9 | |
| 0.00 | 1.20 | 0.00 | 3.01 | -12.82 | 241.43 | 77.95 | 256.60 | 0.9812 | -196.0 | -137.9 | |
| 4.11 | 273.01 | 10.25 | 703.49 | -14.50 | 241.29 | 77.80 | 254.88 | 0.9811 | -424.2 | -56.3 | |
| 5.82 | -3.00 | 15.83 | -3.00 | -15.45 | 242.22 | 78.74 | 253.99 | 0.9843 | -128.3 | 999999 | |
| 2.83 | -3.00 | 6.91 | -3.00 | -14.89 | 241.03 | 77.55 | 254.46 | 0.9804 | -522.8 | 999999 | |
| 0.00 | 1.20 | 0.00 | 2.74 | -14.84 | 240.12 | 76.64 | 254.44 | 0.9773 | -356.0 | -312.4 | |
| 6.59 | -3.00 | 15.92 | -3.00 | -15.65 | 240.68 | 77.20 | 253.66 | 0.9795 | -328.4 | 999999 | |
| 14.99 | -3.00 | 39.22 | -3.00 | -16.95 | 241.55 | 78.07 | 252.41 | 0.9827 | -172.8 | 999999 | |
| 0.26 | -3.00 | 0.59 | -3.00 | -16.63 | 239.97 | 76.49 | 252.60 | 0.9773 | -362.7 | 999999 | |
| 1.20 | -3.00 | 2.81 | -3.00 | -16.94 | 240.24 | 76.76 | 252.30 | 0.9784 | -230.7 | 999999 | |
| 9.33 | -3.00 | 20.44 | -3.00 | -16.76 | 239.34 | 75.86 | 252.40 | 0.9751 | -702.5 | 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. | |