Results 41 to 50 of about 16,482 (212)

The Effect of Steady Flow on the Physical Quantities of Slow mMagneto Acoustic Waves in Solar Coronal Plasma [PDF]

Iranian Journal of Astronomy and Astrophysics, 2020
textbf{Damping of slow magnetohydrodynamic(MHD) waves and oscillations are believed to contribute to the heating of the solar corona. Since the launch of solar space telescopes, many observational evidences for the occurrence of slow MHD waves have been ...
Abbas Abedini
doaj   +1 more source

Connecting the Sun and the Solar Wind: The First 2.5 Dimensional Self-consistent MHD Simulation under the Alfv\'en Wave Scenario

, 2012
The solar wind emanates from the hot and tenuous solar corona. Earlier studies using 1.5 dimensional simulations show that Alfv\'{e}n waves generated in the photosphere play an important role in coronal heating through the process of non-linear mode ...
Antolin, Banerjee, Bogdan, Cranmer, Dmitruk, Einaudi, Esser, Fedun, Hasan, Heyvaerts, Kudoh, Lamy, Matsumoto, Matsumoto, Matthaeus, Nishizuka, Okamoto, Perez, Steiner, Suzuki, Takeru Ken Suzuki, Takuma Matsumoto, Teriaca, Tsuneta, Van Ballegooijen, Verdini, Wilhelm, Yokoyama, Zangrilli   +28 more
core   +1 more source

Spaceborne and spaceborn: Physiological aspects of pregnancy and birth during interplanetary flight

Experimental Physiology, EarlyView.
Abstract Crewed interplanetary return missions that are on the planning horizon will take years, more than enough time for initiation and completion of a pregnancy. Pregnancy is viewed as a sequence of processes – fertilization, blastocyst formation, implantation, gastrulation, placentation, organogenesis, gross morphogenesis, birth and neonatal ...
Arun V. Holden
wiley   +1 more source

THREE-DIMENSIONAL PROPAGATION OF MAGNETOHYDRODYNAMIC WAVES IN SOLAR CORONAL ARCADES [PDF]

The Astrophysical Journal, 2010
We numerically investigate the excitation and temporal evolution of oscillations in a two-dimensional coronal arcade by including the three-dimensional propagation of perturbations. The time evolution of impulsively generated perturbations is studied by solving the linear, ideal magnetohydrodynamic (MHD) equations in the zero-beta approximation.
Rial, S., Arregui, I., Terradas, J., Oliver, R., Ballester, J. L.   +4 more
openaire   +2 more sources

Estimating the Poynting Flux of Alfvénic Waves in Polar Coronal Holes across Solar Cycle 24

The Astrophysical Journal
Alfvénic waves are known to be prevalent throughout the corona and solar wind. Determining the Poynting flux supplied by the waves is required for constraining their role in plasma heating and acceleration, as well as providing a constraint for Alfvén ...
R. J. Morton, M. J. Weberg, N. Balodhi, J. A. McLaughlin   +3 more
doaj   +1 more source

Coronal Shock Waves, EUV waves, and Their Relation to CMEs. I. Reconciliation of "EIT waves", Type II Radio Bursts, and Leading Edges of CMEs

, 2011
We show examples of excitation of coronal waves by flare-related abrupt eruptions of magnetic rope structures. The waves presumably rapidly steepened into shocks and freely propagated afterwards like decelerating blast waves that showed up as Moreton ...
A. Klassen, A. M. Uralov, A. N. Afanasyev, A. Vourlidas, A. Warmuth, A. Warmuth, A. Warmuth, A. Warmuth, A. Warmuth, A.M. Uralov, A.M. Veronig, A.M. Veronig, A.N. Afanasyev, A.N. Zhukov, A.N. Zhukov, B. Filippov, B. Filippov, B. Vršnak, B. Vršnak, B.C. Low, B.C. Low, B.J. Thompson, B.J. Thompson, B.J. Thompson, B.N. Handy, C. Delannée, C. Torii, D.A. Biesecker, D.M. Long, E.W. Cliver, G. Mann, G. Newkirk Jr., G.D.R. Attrill, G.E. Brueckner, G.E. Moreton, G.V. Rudenko, G.V. Rudenko, H. Nakajima, H.Q. Yang, H.S. Hudson, H.S. Hudson, H.V. Cane, I. M. Chertok, I. V. Kuzmenko, I.M. Chertok, I.M. Chertok, J. Magdalenić, J. Magdalenić, J. Pomoell, J.-P. Delaboudinière, J.I. Khan, J.M. Schmidt, K. Ichimoto, K. Saito, L.D. Landau, M. Temmer, M.J. Reiner, M.J. Wills-Davey, M.J. Wills-Davey, M.L. Kaiser, N. Gopalswamy, N. S. Meshalkina, N.R. Sheeley Jr., N.S. Meshalkina, O. Cohen, P.F. Chen, P.T. Gallagher, R.A. Howard, R.P. Lin, S. Mancuso, S. Mancuso, S. Pohjolainen, S. S. Kalashnikov, S. Yashiro, S.M. White, S.V. Uralova, V. V. Grechnev, V.V. Grechnev, V.V. Grechnev, V.V. Grechnev, V.V. Grechnev, V.V. Grechnev, V.V. Zheleznyakov, Y. Kubo, Y. Uchida, Y. Uchida, Y. Wang   +86 more
core   +1 more source

Solar Wind‐Magnetosphere‐Ionosphere Coupling During the October 2024 Storms

Journal of Geophysical Research: Space Physics, Volume 131, Issue 5, May 2026.
Abstract Two geomagnetic storms occurred in October 2024 (Oct 6‐9 and 10–12), driven by the impact of a series of interplanetary coronal mass ejections on the magnetosphere. The first was a moderate storm, with peak Sym‐H near −150 nT, whereas the second was intense, Sym‐H reaching −340 nT.
S. E. Milan, M. K. Mooney, G. E. Bower, R. M. Hodnett, U. V. Amerstorfer, C. Möstl, A. Samsonov, B. J. Anderson, J. Gjerloev, S. K. Vines   +9 more
wiley   +1 more source

Solar wind and kinetic heliophysics [PDF]

Annales Geophysicae, 2018
This paper reviews recent aspects of solar wind physics and elucidates the role Alfvén waves play in solar wind acceleration and turbulence, which prevail in the low corona and inner heliosphere.
E. Marsch, E. Marsch
doaj   +1 more source

Evolution of Magnetospheric Boundary Layers Under the 10 May 2024 ICME Impact

Geophysical Research Letters, Volume 53, Issue 8, 28 April 2026.
Abstract On 10 May 2024, an interplanetary coronal mass ejection‐driven shock impacted the dayside magnetopause, compressing it to ∼5 RE. A northward interplanetary magnetic field suppressed dayside reconnection and allowed a clear investigation of the magnetosphere response.
Sheng Li, Gilbert Pi, Zdeněk Němeček, Jana Šafránková, Trevor W. Leonard, Yang‐Yi Sun   +5 more
wiley   +1 more source

MHD Waves and Oscillations in Solar Coronal Waveguides [PDF]

, 2018
Perturbations of coronal structures by impulsive events such as solar flares generate waves which are interpreted with MHD theory. These waves allow plasma processes to be studied, and seismology of the local plasma parameters to be performed.
openaire   +1 more source