SDO HMI 2014-06-05 02:00:39 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 |
| 58.16 | 311.55 | 28.94 | 154.98 | -4.52 | 301.36 | -2.41 | 151.70 | 0.0876 | 674.6 | 393.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-06-05 02:00:39 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 | 1.18 | 0.00 | 0.59 | -6.82 | 304.35 | 0.58 | 184.95 | 0.1163 | 831.0 | 636.6 | |
| 0.00 | 0.99 | 0.00 | 0.49 | -1.55 | 303.68 | -0.09 | 176.20 | 0.0237 | 867.0 | 609.9 | |
| 3.62 | 7.87 | 1.80 | 3.92 | -5.48 | 302.79 | -0.98 | 169.51 | 0.0940 | 1163.7 | 774.6 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -8.11 | 302.72 | -1.05 | 172.48 | 0.1394 | 909.0 | 629.6 | |
| 3.17 | 5.25 | 1.58 | 2.61 | -5.44 | 302.42 | -1.35 | 165.64 | 0.0948 | 1227.7 | 917.3 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -5.63 | 301.87 | -1.90 | 160.79 | 0.1006 | 1071.0 | 811.8 | |
| 8.50 | 249.38 | 4.23 | 123.94 | -4.44 | 301.81 | -1.95 | 155.30 | 0.0817 | 1361.9 | 425.2 | |
| 32.83 | -7.00 | 16.32 | -7.00 | -4.13 | 301.63 | -2.14 | 151.54 | 0.0784 | 1444.9 | 999999 | |
| 1.09 | -7.00 | 0.54 | -7.00 | -4.59 | 301.51 | -2.26 | 152.82 | 0.0864 | 893.3 | 999999 | |
| 1.63 | -7.00 | 0.81 | -7.00 | -4.01 | 301.21 | -2.56 | 146.13 | 0.0804 | 1035.8 | 999999 | |
| 1.90 | 11.31 | 0.95 | 5.63 | -5.90 | 301.17 | -2.60 | 155.55 | 0.1096 | 1164.6 | 806.9 | |
| 0.54 | -7.00 | 0.27 | -7.00 | -3.83 | 301.12 | -2.65 | 143.87 | 0.0787 | 838.7 | 999999 | |
| 2.08 | 3.35 | 1.04 | 1.67 | -6.14 | 300.83 | -2.94 | 153.78 | 0.1160 | 1082.3 | 802.4 | |
| 2.80 | 9.50 | 1.40 | 4.74 | -5.87 | 300.55 | -3.21 | 150.55 | 0.1140 | 1162.5 | 797.7 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -6.11 | 300.28 | -3.49 | 149.56 | 0.1201 | 735.0 | 671.1 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -5.65 | 299.82 | -3.95 | 144.22 | 0.1177 | 746.0 | 525.3 | |
| 0.00 | 1.72 | 0.00 | 0.86 | -4.68 | 299.67 | -4.09 | 137.67 | 0.1061 | -1013.0 | -784.1 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -7.70 | 297.86 | -5.91 | 142.01 | 0.1665 | -816.0 | -652.8 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -4.92 | 297.74 | -6.03 | 128.20 | 0.1337 | -908.0 | -653.1 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -6.32 | 297.48 | -6.29 | 134.43 | 0.1531 | -1001.0 | -894.3 | |
| 0.00 | 1.54 | 0.00 | 0.78 | -9.70 | 297.33 | -6.44 | 146.20 | 0.1996 | -676.0 | -519.8 | |
| 0.00 | 1.54 | 0.00 | 0.78 | -8.71 | 297.26 | -6.51 | 142.88 | 0.1866 | -1002.0 | -777.7 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -6.63 | 297.23 | -6.54 | 134.72 | 0.1599 | -996.0 | -874.7 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -6.60 | 297.01 | -6.75 | 133.66 | 0.1622 | -942.0 | -748.3 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -5.92 | 296.59 | -7.18 | 128.77 | 0.1601 | -868.0 | -692.0 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -4.85 | 295.71 | -8.05 | 120.18 | 0.1622 | -813.0 | -520.8 | |
| 0.00 | 0.72 | 0.00 | 0.36 | -3.88 | 295.11 | -8.66 | 113.14 | 0.1641 | -866.0 | -701.2 | |
| 0.00 | 2.26 | 0.00 | 1.14 | -4.06 | 295.02 | -8.75 | 113.94 | 0.1668 | -1040.0 | -806.2 | |
| 0.00 | 0.72 | 0.00 | 0.36 | -4.33 | 294.92 | -8.85 | 115.19 | 0.1703 | -823.0 | -652.6 | |
| 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. | |