SDO HMI 2014-09-26 17:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.56 | 20.84 | 2.50 | 20.54 | -14.53 | 185.04 | -56.33 | 111.27 | 0.8663 | -46.4 | -71.0 | |
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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 | 1.32 | 0.00 | 1.25 | -14.47 | 186.73 | -54.65 | 111.77 | 0.8525 | 515.0 | 415.0 | |
| 0.00 | 1.94 | 0.00 | 1.80 | -13.56 | 186.94 | -54.43 | 110.82 | 0.8481 | 694.0 | 459.0 | |
| 0.79 | 1.85 | 0.75 | 1.75 | -14.26 | 186.59 | -54.79 | 111.49 | 0.8531 | 388.6 | 356.7 | |
| 0.00 | 0.53 | 0.00 | 0.49 | -13.41 | 186.83 | -54.54 | 110.62 | 0.8486 | 515.0 | 490.8 | |
| 0.00 | 0.79 | 0.00 | 0.75 | -14.09 | 186.38 | -55.00 | 111.23 | 0.8544 | 423.0 | 405.7 | |
| 0.00 | 1.15 | 0.00 | 1.09 | -13.21 | 186.04 | -55.34 | 110.12 | 0.8549 | 308.0 | 273.4 | |
| 0.71 | 1.24 | 0.67 | 1.18 | -13.10 | 185.80 | -55.58 | 109.93 | 0.8566 | 370.9 | 330.3 | |
| 1.06 | 2.74 | 1.08 | 2.79 | -15.72 | 184.21 | -57.17 | 112.30 | 0.8762 | -480.2 | -425.9 | |
| 0.00 | 1.15 | 0.00 | 1.13 | -13.95 | 184.93 | -56.44 | 110.60 | 0.8660 | -508.0 | -444.5 | |
| 0.00 | 0.71 | 0.00 | 0.72 | -15.45 | 184.04 | -57.34 | 111.95 | 0.8769 | -521.0 | -459.8 | |
| 0.00 | 1.50 | 0.00 | 1.54 | -15.53 | 183.95 | -57.43 | 112.00 | 0.8777 | -316.0 | -193.3 | |
| 0.00 | 0.53 | 0.00 | 0.54 | -15.26 | 184.06 | -57.31 | 111.75 | 0.8762 | -559.0 | -488.7 | |
| 0.00 | 2.30 | 0.00 | 2.34 | -14.85 | 184.00 | -57.37 | 111.28 | 0.8756 | -460.0 | -363.6 | |
| 0.00 | 0.97 | 0.00 | 1.00 | -14.79 | 183.68 | -57.70 | 111.11 | 0.8780 | -267.0 | -227.2 | |
| 0.00 | 2.12 | 0.00 | 2.17 | -14.59 | 183.70 | -57.67 | 110.90 | 0.8773 | -518.0 | -365.8 | |
| 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. | |