SDO HMI 2014-09-13 14:00:35 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 |
| 86.82 | 440.00 | 61.99 | 312.95 | -14.79 | 95.11 | 40.48 | 241.06 | 0.7187 | -270.4 | -150.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-13 14:00:35 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 |
| 2.85 | 11.56 | 2.37 | 9.64 | -11.85 | 104.91 | 50.28 | 249.45 | 0.8062 | 709.7 | 547.5 | |
| 1.42 | 4.54 | 1.16 | 3.71 | -12.38 | 103.89 | 49.26 | 248.42 | 0.7981 | 757.3 | 621.9 | |
| 0.00 | 1.16 | 0.00 | 0.95 | -12.81 | 104.01 | 49.37 | 247.96 | 0.8007 | 477.0 | 422.1 | |
| 0.00 | 1.78 | 0.00 | 1.50 | -14.93 | 104.43 | 49.80 | 245.66 | 0.8122 | 263.0 | 260.0 | |
| 0.00 | 1.51 | 0.00 | 1.21 | -11.90 | 103.21 | 48.58 | 248.71 | 0.7897 | 614.0 | 466.0 | |
| 0.00 | 3.38 | 0.00 | 2.68 | -11.23 | 102.77 | 48.14 | 249.35 | 0.7830 | 47.0 | 88.3 | |
| 0.00 | 0.89 | 0.00 | 0.71 | -13.45 | 102.43 | 47.80 | 246.54 | 0.7877 | 572.0 | 519.0 | |
| 0.00 | 0.98 | 0.00 | 0.79 | -15.25 | 102.43 | 47.80 | 244.41 | 0.7947 | 402.0 | 367.3 | |
| 0.00 | 0.80 | 0.00 | 0.62 | -12.96 | 101.03 | 46.40 | 246.50 | 0.7718 | 326.0 | 420.4 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -12.75 | 100.44 | 45.81 | 246.49 | 0.7650 | 614.0 | 578.6 | |
| 0.00 | 0.89 | 0.00 | 0.69 | -17.12 | 99.21 | 44.58 | 240.63 | 0.7720 | 295.0 | 335.7 | |
| 0.00 | 0.89 | 0.00 | 0.65 | -12.62 | 97.72 | 43.09 | 245.32 | 0.7359 | -417.0 | -402.4 | |
| 0.00 | 3.82 | 0.00 | 2.78 | -12.29 | 97.61 | 42.98 | 245.68 | 0.7332 | -597.0 | -551.4 | |
| 3.20 | 5.78 | 2.34 | 4.22 | -13.06 | 97.68 | 43.05 | 244.75 | 0.7376 | -692.2 | -566.9 | |
| 0.00 | 0.89 | 0.00 | 0.64 | -12.09 | 97.44 | 42.81 | 245.86 | 0.7305 | -422.0 | -413.5 | |
| 6.23 | 9.52 | 4.68 | 7.15 | -15.61 | 98.08 | 43.45 | 241.83 | 0.7537 | 617.9 | 307.5 | |
| 3.29 | 5.43 | 2.41 | 3.97 | -13.50 | 97.52 | 42.89 | 244.12 | 0.7379 | -629.4 | -421.6 | |
| 0.00 | 0.89 | 0.00 | 0.66 | -14.32 | 97.71 | 43.08 | 243.21 | 0.7437 | 675.0 | 523.2 | |
| 0.00 | 0.71 | 0.00 | 0.54 | -17.04 | 98.05 | 43.41 | 240.09 | 0.7603 | 419.0 | 343.5 | |
| 0.00 | 0.44 | 0.00 | 0.33 | -15.60 | 97.61 | 42.97 | 241.58 | 0.7488 | 522.0 | 499.4 | |
| 0.00 | 2.76 | 0.00 | 1.99 | -13.08 | 96.80 | 42.17 | 244.27 | 0.7282 | -655.0 | -487.5 | |
| 0.00 | 1.33 | 0.00 | 1.00 | -16.25 | 97.56 | 42.93 | 240.78 | 0.7516 | 506.0 | 421.0 | |
| 0.00 | 1.51 | 0.00 | 1.12 | -15.68 | 97.41 | 42.78 | 241.38 | 0.7472 | 595.0 | 431.6 | |
| 0.00 | 1.25 | 0.00 | 0.90 | -13.99 | 96.54 | 41.90 | 242.98 | 0.7298 | -428.0 | -316.2 | |
| 8.54 | 31.48 | 6.20 | 22.88 | -15.00 | 96.35 | 41.72 | 241.62 | 0.7330 | 776.1 | 589.2 | |
| 2.67 | 48.38 | 1.93 | 34.77 | -15.88 | 95.64 | 41.01 | 240.12 | 0.7302 | 601.8 | 55.1 | |
| 0.80 | -26.00 | 0.58 | -26.00 | -16.07 | 95.61 | 40.98 | 239.87 | 0.7309 | 391.2 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -16.80 | 95.71 | 41.08 | 239.04 | 0.7359 | 579.0 | 479.3 | |
| 1.42 | -26.00 | 1.02 | -26.00 | -16.19 | 95.14 | 40.51 | 239.44 | 0.7268 | -440.8 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.50 | -15.44 | 94.71 | 40.08 | 240.11 | 0.7182 | -562.0 | -469.0 | |
| 3.38 | -26.00 | 2.42 | -26.00 | -16.27 | 94.83 | 40.20 | 239.16 | 0.7239 | -492.1 | 999999 | |
| 3.65 | 274.20 | 2.56 | 190.76 | -14.87 | 94.42 | 39.79 | 240.65 | 0.7119 | -595.1 | -322.3 | |
| 23.30 | -32.00 | 16.24 | -32.00 | -14.57 | 93.99 | 39.36 | 240.76 | 0.7057 | -898.1 | 999999 | |
| 0.00 | 1.96 | 0.00 | 1.38 | -15.93 | 94.29 | 39.66 | 239.25 | 0.7165 | 361.0 | 209.6 | |
| 1.25 | -32.00 | 0.87 | -32.00 | -15.21 | 93.88 | 39.25 | 239.89 | 0.7082 | -392.7 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.78 | -11.11 | 93.07 | 38.44 | 244.75 | 0.6768 | -635.0 | -532.3 | |
| 3.65 | -32.00 | 2.57 | -32.00 | -16.03 | 93.95 | 39.32 | 238.91 | 0.7135 | 693.2 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.88 | -16.49 | 94.02 | 39.39 | 238.38 | 0.7169 | -585.0 | -519.5 | |
| 0.89 | -32.00 | 0.61 | -32.00 | -14.43 | 93.52 | 38.89 | 240.64 | 0.6998 | -1006.8 | 999999 | |
| 1.07 | -32.00 | 0.75 | -32.00 | -15.38 | 93.64 | 39.01 | 239.52 | 0.7066 | -328.0 | 999999 | |
| 19.21 | -32.00 | 13.28 | -32.00 | -14.77 | 93.31 | 38.68 | 240.08 | 0.6995 | -1092.9 | 999999 | |
| 0.00 | 0.36 | 0.00 | 0.24 | -13.31 | 92.74 | 38.11 | 241.61 | 0.6849 | -590.0 | -560.8 | |
| 0.00 | 2.58 | 0.00 | 1.80 | -16.78 | 92.79 | 38.16 | 237.22 | 0.7059 | -579.0 | -439.8 | |
| 0.00 | 0.71 | 0.00 | 0.51 | -18.39 | 93.12 | 38.49 | 235.47 | 0.7191 | -542.0 | -471.0 | |
| 0.00 | 1.07 | 0.00 | 0.74 | -16.89 | 92.50 | 37.87 | 236.89 | 0.7035 | -535.0 | -429.0 | |
| 0.00 | 2.49 | 0.00 | 1.72 | -16.55 | 92.42 | 37.79 | 237.25 | 0.7007 | -656.0 | -468.7 | |
| 0.00 | 1.07 | 0.00 | 0.74 | -16.59 | 92.07 | 37.44 | 236.97 | 0.6972 | -458.0 | -448.0 | |
| 0.00 | 2.40 | 0.00 | 1.58 | -12.32 | 91.20 | 36.57 | 241.94 | 0.6619 | -708.0 | -619.5 | |
| 0.00 | 3.02 | 0.00 | 2.13 | -18.46 | 92.32 | 37.69 | 234.85 | 0.7116 | -110.0 | -172.6 | |
| 0.00 | 0.71 | 0.00 | 0.50 | -20.15 | 91.81 | 37.18 | 232.47 | 0.7176 | -555.0 | -458.5 | |
| 0.00 | 1.51 | 0.00 | 1.00 | -16.27 | 89.31 | 34.68 | 235.38 | 0.6660 | -620.0 | -457.6 | |
| 0.00 | 0.98 | 0.00 | 0.65 | -16.16 | 89.06 | 34.43 | 235.33 | 0.6625 | -668.0 | -495.5 | |
| 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. | |