Results 1 to 10 of about 36,388 (256)

On the Existence of Long-period Decayless Oscillations in Short Active Region Loops

open access: yesThe Astrophysical Journal
Decayless kink oscillations, characterized by their lack of decay in amplitude, have been detected in coronal loops of varying scales in active regions, the quiet Sun, and coronal holes. Short-period (
Arpit Kumar Shrivastav   +7 more
doaj   +1 more source

Sources of magnetic fields in recurrent interplanetary streams [PDF]

open access: yes
The sources of magnetic fields in recurrent streams were examined. Most fields and plasmas at 1 AU were related to coronal holes, and the magnetic field lines were open in those holes.
Behannon, K. W.   +4 more
core   +1 more source

Preferential energization of alpha particles in polar coronal holes at one solar radius above the photosphere

open access: yes, 2015
Heating of polar coronal holes during solar minimum and acceleration of the fast solar wind issuing therefrom lack comprehensive theoretical understanding.
Bose, M., Chakravarty, Aniruddha
core   +1 more source

On the Origin of the Sudden Heliospheric Open Magnetic Flux Enhancement During the 2014 Pole Reversal

open access: yesThe Astrophysical Journal
Coronal holes are recognized as the primary sources of heliospheric open magnetic flux (OMF). However, a noticeable gap exists between in situ measured OMF and that derived from remote-sensing observations of the Sun.
Stephan G. Heinemann   +14 more
doaj   +1 more source

Effect of coronal temperature on the scale of solar chromospheric jets

open access: yes, 2015
We investigate the effect of coronal temperature on the formation process of solar chromospheric jets using two-dimensional magnetohydrodynamic simulations of the region from the upper convection zone to the lower corona.
Iijima, H., Yokoyama, T.
core   +1 more source

What drives solar-EUV jets seen in equatorial coronal holes?

open access: yesResults in Physics, 2016
Recent observations of jets in solar coronal holes that include multi-wavelength data such as EUV movies have shown that most of those jets are not driven in the way suggested by the standard model.
M.L. Adams, R.L. Moore
doaj   +1 more source

Soft X-ray telescope (SXRT) [PDF]

open access: yes
The soft X-ray telescope (SXRT) will provide direct images of the solar corona with spatial resolution of about 1 arcsecond. These images will show the global structure of the corona, the location and area of coronal holes, and the presence of even the ...
Moore, R.
core   +4 more sources

Hydrogen Lyman-alpha and Lyman-beta radiances and profiles in polar coronal holes

open access: yes, 2009
The hydrogen Lyman-alpha plays a dominant role in the radiative energy transport in the lower transition region, and is important for the stud- ies of transition-region structure as well as solar wind origin. We investigate the Ly-alpha profiles obtained
Dammasch   +12 more
core   +1 more source

JETS IN POLAR CORONAL HOLES

open access: yesThe Astrophysical Journal, 2009
Here, we explore the nature of small-scale jet-like structures and their possible relation to explosive events and other known transient features, like spicules and macrospicules, using high-resolution spectroscopy obtained with the Solar and Heliospheric Observatory/Solar Ultraviolet Measurements of Emitted Radiation instrument.
E. Scullion   +4 more
openaire   +1 more source

Observations of coronal holes with the Siberian Radioheliograph

open access: yesSolar-Terrestrial Physics
Multi-wavelength observations of a coronal hole (CH) with two-dimensional spatial resolution have been made for the first time in the frequency range from 2.8 to 12 GHz.
Globa M. V.   +2 more
doaj   +1 more source

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