The National Science Foundation’s (NSF) Daniel K. Onauye Solar Telencope, located in the Summit of Haleakalā on the Island of Maui, Hawaii, captured the sharp-face image of the sun.
Images shows ultra-finay bright and dark stripes (called striations) in thin, gas layer of DAY emptiness known as Photosphere, according to a statement From the National Solar Ofnofvatory (NSO), acting on the solar telescope.
“In this work, we have reviewed the good structure of solar face For the first time there has been no more spatial resolution of about 20 miles (12.4.4 miles), “David Kuridips, the centers of Nos,” These are the centers of the Nos-scale magnetic field. “
Leases appear as polished bright and dark straps along the walls of the solar granules – cells cells shining warmth from the sunlight. These patterns result from curtain Magnetic Field that ripple and transfer like cloth flowing into the air.
As the light from hot granule walls passing through magnets “curtains,” differences in magnetic fields are causing changes to the changes in magnets. If the magnetic fiels are weaker than its surroundings, it is darker; If stronger, it shines in light.
Therefore, the declines are believed to sign the signatures of bad magnetic changes, changing the density and opacity of solar plasma. These slight moves see only thanks to the telescope Visible Dirure of Broadband (VBI)moving on the G-Band – a specified order of visible lighting lighting places with strong magnetic activity.
Magnetic architectural unrelling is the key to understanding events like Solar Flaresblasts and coronal mass ejections (cmes), driving during space and affect the land.
The teams found Published May 20 In letters in the Asstrophysical Journal.
