SDO HMI 2014-06-30 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.54 | 36.86 | 22.32 | 47.58 | 14.22 | 258.31 | -67.41 | 75.74 | 0.9243 | -241.4 | -144.9 | |
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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 | 1.09 | 0.00 | 1.14 | 12.47 | 263.98 | -61.74 | 77.35 | 0.8833 | -556.0 | -516.4 | |
| 0.91 | 9.81 | 1.05 | 11.31 | 15.36 | 261.30 | -64.41 | 74.31 | 0.9051 | -480.2 | -390.1 | |
| 5.09 | -2.00 | 5.86 | -2.00 | 15.11 | 261.30 | -64.42 | 74.59 | 0.9050 | -512.7 | 999999 | |
| 1.09 | 2.45 | 1.31 | 2.95 | 15.88 | 260.16 | -65.56 | 73.83 | 0.9134 | -183.3 | -154.1 | |
| 0.00 | 0.27 | 0.00 | 0.33 | 14.68 | 259.96 | -65.76 | 75.16 | 0.9142 | -393.0 | -353.0 | |
| 0.00 | 0.64 | 0.00 | 0.80 | 14.01 | 259.01 | -66.71 | 75.95 | 0.9203 | -317.0 | -297.3 | |
| 0.00 | 1.18 | 0.00 | 1.58 | 14.76 | 257.54 | -68.17 | 75.21 | 0.9300 | 471.0 | 535.4 | |
| 3.00 | 4.90 | 4.06 | 6.63 | 15.00 | 257.21 | -68.51 | 74.98 | 0.9321 | 389.4 | 327.8 | |
| 7.45 | 10.08 | 10.04 | 13.58 | 13.40 | 257.20 | -68.51 | 76.70 | 0.9317 | -337.0 | -154.8 | |
| 0.00 | 1.36 | 0.00 | 1.83 | 13.09 | 257.30 | -68.42 | 77.02 | 0.9310 | -569.0 | -479.6 | |
| 0.00 | 1.36 | 0.00 | 1.82 | 12.91 | 257.41 | -68.31 | 77.22 | 0.9303 | -433.0 | -353.0 | |
| 0.00 | 1.09 | 0.00 | 1.49 | 12.85 | 256.84 | -68.88 | 77.30 | 0.9338 | -193.0 | -155.8 | |
| 0.00 | 1.54 | 0.00 | 2.27 | 13.65 | 255.22 | -70.50 | 76.50 | 0.9435 | -370.0 | -295.8 | |
| 0.00 | 1.09 | 0.00 | 1.85 | 13.91 | 252.58 | -73.14 | 76.30 | 0.9574 | 351.0 | 291.3 | |
| 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. | |