Приклади вживання Coronal Англійська мовою та їх переклад на Українською
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Rotation of active regions and coronal holes from observations of the Sun in the line He I λ 1083 nm.
Solar wind flowing from this coronal hole should reach Earth on July 20-21.
contain plasma less dense than in the coronal loops of the active regions.
After analyzing the data it was found that this had a coronal mass ejection rate between 2880 and 3520 km/ s.
This caused the first of two coronal mass ejections(CMEs),
The E-corona(E for emission) is due to spectral emission lines produced by ions that are present in the coronal plasma;
the record coronal mass ejection brought to STEREO
Many scales of coronal loops exist, neighbouring open flux tubes
A stream of solar wind flowing from the indicated coronal hole should reach Earth on July 19-20.
highly dynamic processes in coronal loops.
On 10/23/02, Earth glided into a solar wind stream flowing from a large coronal hole.
The black area to the left of the brighter active region is a coronal hole, a magnetically open region of the sun.".
These loops are the closed-magnetic flux cousins of the open-magnetic flux that can be found in coronal hole(polar) regions
The most dramatic difference in these three parameters occur when the solar wind escapes from a coronal hole or as a coronal mass ejection.
The above shot taken with the WISPR instrument shows a coronal streamer with Mercury visible as the bright dot.
charged particles of high energy and emissions of the coronal solar mass.
as they are sensitive to the radiation emitted by quiescent coronal loops.
Like the hole in the ozone layer on Earth, a coronal hole doesn't actually go through the sun's atmosphere.
A geomagnetic storm is thus the result of a coronal hole solar wind stream or a coronal mass ejection arriving at Earth.
An example occurred in mid-July 2012 after an eruption on the Sun that produced both a Coronal Mass Ejection