SDO HMI 2014-07-08 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.15 | 137.20 | 33.11 | 220.49 | -19.33 | 149.78 | -68.94 | 111.79 | 0.9496 | 373.0 | -47.0 | |
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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 | 2.63 | 0.00 | 3.92 | -20.00 | 150.99 | -67.74 | 112.72 | 0.9442 | 365.0 | 283.3 | |
| 1.63 | 79.90 | 2.56 | 130.76 | -20.14 | 149.89 | -68.84 | 112.64 | 0.9500 | 307.1 | -156.5 | |
| 0.00 | 3.54 | 0.00 | 4.61 | -15.62 | 153.24 | -65.49 | 108.56 | 0.9260 | 535.0 | 429.1 | |
| 14.16 | -2.00 | 22.29 | -2.00 | -19.69 | 149.67 | -69.05 | 112.14 | 0.9506 | 406.0 | 999999 | |
| 3.45 | 46.94 | 5.27 | 73.80 | -18.59 | 150.04 | -68.68 | 111.07 | 0.9476 | 769.6 | 93.9 | |
| 1.91 | -5.00 | 2.99 | -5.00 | -19.07 | 149.61 | -69.11 | 111.49 | 0.9503 | 413.4 | 999999 | |
| 0.00 | 1.00 | 0.00 | 1.62 | -19.30 | 149.02 | -69.70 | 111.62 | 0.9535 | 116.0 | 71.9 | |
| 0.00 | 0.82 | 0.00 | 1.35 | -19.22 | 148.72 | -70.01 | 111.48 | 0.9549 | -296.0 | -260.2 | |
| 0.00 | 0.64 | 0.00 | 1.07 | -19.35 | 148.20 | -70.53 | 111.52 | 0.9575 | -247.0 | -232.3 | |
| 0.00 | 0.91 | 0.00 | 1.72 | -20.82 | 146.37 | -72.35 | 112.71 | 0.9667 | -254.0 | -246.4 | |
| 0.00 | 0.82 | 0.00 | 1.64 | -19.50 | 145.27 | -73.45 | 111.19 | 0.9702 | -385.0 | -341.4 | |
| 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. | |