-
surrounding medium by
magnetic flux tubes.
Coronal loops begin and end at two
footpoints on the
photosphere and
project into the
transition region and
lower corona...
- helio-latitude, as the
speed of the
photospheric footpoint is reduced.
Depending on the
polarity of the
photospheric footpoint, the
heliospheric magnetic field spirals...
-
appears in
patches spanning 6,000-12,000 miles,
typically found at the
footpoints of high-pressure
coronal loops in
active regions.
While moss formations...
-
Emerging magnetic flux and
photospheric motions continuously shifting the
footpoints of a
structure can
result in
magnetic free
energy building up in the coronal...
- dawn to dusk.
Along the last
closed geomagnetic field lines with
their footpoints within the
auroral zones, field-aligned
electric currents can flow into...
- 2013-01-24. Kat****wa, Yukio; Tsuneta, Saku (2005). "Magnetic
Properties at
Footpoints of Hot and Cool Loops". The
Astrophysical Journal. 621 (1): 498–511. Bibcode:2005ApJ...
-
algorithm uses time-consuming
procedures like the
determination of the
footpoint of a
perpendicular on a surface. The
second part of the
marching method...
- the
polar magnetosphere with open
magnetic fieldlines (having only one
footpoint on Earth), and τ the
local time. θm ~ 20° is the
polar border of the auroral...
-
magnetic flux
tubes that are
attached to the photosphere,
referred to as
footpoints,
create a loop-like
structure known as a
coronal loop. The
plasma inside...
- (help) Kat****wa, Yukio; Tsuneta, Saku (2005). "Magnetic
Properties at
Footpoints of Hot and Cool Loops". The
Astrophysical Journal. 621 (1): 498–511. Bibcode:2005ApJ...
