Results 111 to 120 of about 3,881 (215)
We examined solar photospheric magnetic fields for the solar cycles 21–25, covering the period 1975–2024. The unsigned photospheric magnetic fields at low latitudes (0°–45°), known as solar toroidal fields, showed a solar cycle variation with the total ...
Harsha Avinash Tanti +3 more
doaj +1 more source
Direct comparison of Viking 2.3-GHz signal phase fluctuation and columnar electron density between 2 and 160 solar radii [PDF]
The relationship between solar wind induced signal phase fluctuation and solar wind columnar electron density has been the subject of intensive analysis during the last two decades.
Berman, A. L. +2 more
core +1 more source
We have conducted a comprehensive comparison of interplanetary scintillation (IPS) observations taken by the Murchison Widefield Array (MWA) with several heliospheric transient event catalogs, over a time period of 7 months during solar minimum.
A. Waszewski +8 more
doaj +1 more source
Three-dimensional exploration of the solar wind using observations of interplanetary scintillation. [PDF]
Tokumaru M.
europepmc +1 more source
Earth-affecting solar transients: a review of progresses in solar cycle 24. [PDF]
Zhang J +18 more
europepmc +1 more source
Precision Magnetometers for Aerospace Applications: A Review. [PDF]
Bennett JS +8 more
europepmc +1 more source
Dynamics of Slow Solar Wind Emerging from an Equatorial Coronal Hole
We present a three-dimensional reduced magnetohydrodynamics model to depict turbulence induced by Alfvén waves within the slow solar wind originating from an open magnetic field positioned in a coronal hole near the solar equator.
M. Asgari-Targhi, K. Fujiki
doaj +1 more source
Ionospheric Plasma IRregularities - IPIR - Data Product Based on Data From the Swarm Satellites. [PDF]
Jin Y +7 more
europepmc +1 more source
Interplanetary Scintillations. II Observations
M. H. Cohen +3 more
openaire +1 more source
Different Polarized Components of the Quasar 3C 286 Revealed by FAST
3C 286, a well-known radio calibrator, exhibits stability in both total flux density and polarization parameters. However, its stable and luminous interstellar radio signal may encounter interplanetary scintillation (IPS) due to density irregularities in
Pengfu Tian +3 more
doaj +1 more source

