SDO HMI 2014-09-14 23:00:35 UT
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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.18 | 127.95 | 15.74 | 87.13 | 12.39 | 352.92 | -43.53 | 79.56 | 0.6852 | -251.3 | -260.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-14 23:00:35 UT
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 | 1.16 | 0.00 | 0.74 | 13.03 | 356.44 | -40.02 | 78.28 | 0.6421 | -763.0 | -607.0 | |
| 0.44 | 2.58 | 0.29 | 1.67 | 13.58 | 355.96 | -40.50 | 77.50 | 0.6489 | -763.0 | -657.6 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 11.36 | 356.09 | -40.36 | 80.91 | 0.6453 | -783.0 | -596.8 | |
| 0.00 | 1.87 | 0.00 | 1.21 | 11.88 | 355.76 | -40.70 | 80.13 | 0.6500 | -933.0 | -823.9 | |
| 0.00 | 2.31 | 0.00 | 1.51 | 12.33 | 355.60 | -40.86 | 79.46 | 0.6524 | -913.0 | -724.3 | |
| 0.00 | 3.20 | 0.00 | 2.09 | 12.63 | 355.54 | -40.92 | 79.00 | 0.6534 | -764.0 | -671.3 | |
| 0.00 | 1.60 | 0.00 | 1.04 | 11.11 | 355.61 | -40.85 | 81.33 | 0.6515 | -775.0 | -655.7 | |
| 0.00 | 2.93 | 0.00 | 1.93 | 12.96 | 355.18 | -41.28 | 78.52 | 0.6583 | -631.0 | -542.3 | |
| 0.00 | 0.98 | 0.00 | 0.64 | 10.80 | 355.50 | -40.96 | 81.82 | 0.6529 | -531.0 | -514.0 | |
| 3.82 | 47.28 | 2.51 | 31.22 | 12.29 | 355.19 | -41.27 | 79.54 | 0.6576 | -939.0 | -318.3 | |
| 0.00 | 1.51 | 0.00 | 0.99 | 10.90 | 355.28 | -41.18 | 81.67 | 0.6558 | -733.0 | -631.5 | |
| 0.00 | 4.62 | 0.00 | 3.03 | 11.19 | 355.10 | -41.36 | 81.23 | 0.6581 | -781.0 | -704.4 | |
| 8.35 | -10.00 | 5.51 | -10.00 | 12.23 | 354.83 | -41.63 | 79.66 | 0.6622 | -867.8 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 11.39 | 354.94 | -41.51 | 80.93 | 0.6603 | -576.0 | -633.6 | |
| 0.71 | -10.00 | 0.47 | -10.00 | 12.42 | 354.54 | -41.91 | 79.40 | 0.6660 | -602.5 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.41 | 10.37 | 354.79 | -41.67 | 82.48 | 0.6619 | -630.0 | -624.4 | |
| 1.07 | -10.00 | 0.71 | -10.00 | 12.17 | 354.43 | -42.03 | 79.79 | 0.6673 | -584.2 | 999999 | |
| 0.00 | 5.07 | 0.00 | 3.35 | 11.48 | 354.56 | -41.90 | 80.82 | 0.6653 | -662.0 | -672.3 | |
| 0.62 | 1.78 | 0.41 | 1.17 | 10.51 | 354.64 | -41.82 | 82.27 | 0.6639 | -718.4 | -585.9 | |
| 0.00 | 0.89 | 0.00 | 0.59 | 11.35 | 354.41 | -42.04 | 81.03 | 0.6670 | -501.0 | -418.6 | |
| 0.00 | 0.89 | 0.00 | 0.59 | 11.20 | 354.44 | -42.02 | 81.25 | 0.6666 | -425.0 | -371.7 | |
| 0.44 | 1.51 | 0.29 | 1.00 | 10.71 | 354.48 | -41.97 | 81.98 | 0.6659 | -686.2 | -554.5 | |
| 0.00 | 0.62 | 0.00 | 0.41 | 10.51 | 354.27 | -42.19 | 82.28 | 0.6686 | -537.0 | -416.4 | |
| 0.71 | 2.58 | 0.47 | 1.72 | 11.80 | 354.00 | -42.46 | 80.37 | 0.6726 | -508.5 | -361.8 | |
| 0.00 | 2.22 | 0.00 | 1.49 | 12.00 | 353.87 | -42.58 | 80.08 | 0.6742 | 247.0 | 204.6 | |
| 0.00 | 1.42 | 0.00 | 0.95 | 10.70 | 353.99 | -42.47 | 82.01 | 0.6723 | -736.0 | -601.1 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 11.78 | 353.79 | -42.67 | 80.41 | 0.6752 | -249.0 | -227.7 | |
| 0.00 | 0.44 | 0.00 | 0.30 | 13.34 | 353.39 | -43.07 | 78.14 | 0.6813 | -366.0 | -304.2 | |
| 0.00 | 0.71 | 0.00 | 0.48 | 12.26 | 353.61 | -42.84 | 79.72 | 0.6777 | 221.0 | 193.0 | |
| 0.00 | 2.49 | 0.00 | 1.67 | 10.80 | 353.72 | -42.74 | 81.87 | 0.6757 | -662.0 | -600.1 | |
| 0.00 | 1.24 | 0.00 | 0.83 | 10.47 | 353.69 | -42.77 | 82.37 | 0.6760 | -432.0 | -366.6 | |
| 0.00 | 1.87 | 0.00 | 1.26 | 10.55 | 353.26 | -43.20 | 82.25 | 0.6815 | -533.0 | -420.0 | |
| 0.00 | 0.71 | 0.00 | 0.50 | 15.48 | 351.15 | -45.31 | 75.31 | 0.7105 | -278.0 | -270.5 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 13.84 | 351.36 | -45.10 | 77.61 | 0.7065 | -408.0 | -335.1 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 10.31 | 351.81 | -44.65 | 82.62 | 0.6996 | -672.0 | -563.1 | |
| 0.00 | 2.13 | 0.00 | 1.53 | 16.18 | 350.04 | -46.41 | 74.47 | 0.7243 | -213.0 | -382.0 | |
| 0.00 | 0.98 | 0.00 | 0.68 | 10.44 | 351.30 | -45.16 | 82.43 | 0.7057 | -326.0 | -309.5 | |
| 0.00 | 0.71 | 0.00 | 0.52 | 17.23 | 349.29 | -47.16 | 73.14 | 0.7342 | -511.0 | -438.0 | |
| 0.00 | 0.62 | 0.00 | 0.45 | 13.73 | 349.78 | -46.68 | 77.89 | 0.7252 | 785.0 | 696.6 | |
| 0.00 | 0.80 | 0.00 | 0.58 | 13.77 | 349.49 | -46.96 | 77.86 | 0.7285 | 622.0 | 512.4 | |
| 6.58 | 12.26 | 4.74 | 8.84 | 13.39 | 349.45 | -47.00 | 78.37 | 0.7287 | 841.8 | 591.4 | |
| 0.00 | 1.24 | 0.00 | 0.91 | 13.12 | 348.74 | -47.71 | 78.79 | 0.7368 | 526.0 | 404.4 | |
| 0.00 | 0.44 | 0.00 | 0.33 | 14.36 | 347.56 | -48.90 | 77.19 | 0.7509 | -388.0 | -372.0 | |
| 0.00 | 1.07 | 0.00 | 0.80 | 13.50 | 347.23 | -49.22 | 78.36 | 0.7541 | 633.0 | 575.5 | |
| 0.44 | 1.33 | 0.34 | 1.02 | 15.31 | 346.50 | -49.96 | 76.02 | 0.7633 | 705.6 | 570.8 | |
| 0.00 | 1.07 | 0.00 | 0.81 | 13.01 | 346.89 | -49.57 | 79.02 | 0.7578 | 422.0 | 384.9 | |
| 0.00 | 1.24 | 0.00 | 0.97 | 14.62 | 345.39 | -51.07 | 76.99 | 0.7748 | 555.0 | 423.8 | |
| 0.00 | 0.53 | 0.00 | 0.42 | 13.75 | 345.31 | -51.15 | 78.12 | 0.7753 | 502.0 | 417.8 | |
| 0.00 | 0.62 | 0.00 | 0.50 | 15.80 | 343.91 | -52.55 | 75.57 | 0.7910 | 464.0 | 455.7 | |
| 0.00 | 0.62 | 0.00 | 0.50 | 15.66 | 343.75 | -52.70 | 75.75 | 0.7925 | 542.0 | 455.3 | |
| 0.00 | 1.24 | 0.00 | 0.99 | 12.20 | 344.25 | -52.20 | 80.13 | 0.7862 | 738.0 | 675.6 | |
| 0.00 | 0.98 | 0.00 | 0.78 | 12.27 | 344.03 | -52.43 | 80.04 | 0.7886 | 709.0 | 625.6 | |
| 0.00 | 0.98 | 0.00 | 0.79 | 11.86 | 343.89 | -52.57 | 80.56 | 0.7900 | 327.0 | 267.7 | |
| 0.00 | 0.44 | 0.00 | 0.37 | 14.98 | 342.43 | -54.03 | 76.68 | 0.8057 | 344.0 | 393.0 | |
| 0.00 | 0.89 | 0.00 | 0.75 | 9.65 | 341.59 | -54.87 | 83.28 | 0.8140 | -564.0 | -438.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |