Results 121 to 130 of about 35,714 (290)

Analysis of fluctuations in the magnetic field obtained by IMP-2 [PDF]

Interplanetary magnetic field fluctuations from IMP 2 ...
Kawashima, N.
core   +1 more source

Rigidity Dependence of the Long-Term Variations of Galactic Cosmic-Ray Intensity in Relation to the Interplanetary Magnetic-Field Turbulence: 1968 – 2002 [PDF]

, 2014
Marek Siłuszyk, K. Iskra, M. V. Alania
openalex   +1 more source

Predicting Dual‐Satellite Ionospheric Radial Currents From Single‐Satellite Observations With a BiLSTM Model

Space Weather, Volume 24, Issue 1, January 2026.
Abstract Ionospheric radial currents (IRC) can be derived using two methodologies: (a) the single‐satellite approach: Single‐IRC is deduced from magnetic field data of a single satellite (Swarm‐A); (b) the dual‐satellite approach: Dual‐IRC is calculated by coordinated magnetic field measurements of a pair of satellites (Swarm‐A and ‐C).
Hao Xia, Hui Wang, Kedeng Zhang, Ming Wang   +3 more
wiley   +1 more source

Solar Wind and Interplanetary Magnetic Field Influence on Ultralow Frequency Waves and Reflected Ions Near the Moon. [PDF]

J Geophys Res Space Phys, 2020
Howard SK, Halekas JS, Farrell WM, McFadden JP, Glassmeier KH.   +4 more
europepmc   +1 more source

The causes of recurrent geomagnetic storms [PDF]

The causes of recurrent geomagnetic activity were studied by analyzing interplanetary magnetic field and plasma data from earth-orbiting spacecraft in the interval from November 1973 to February 1974.
Burlaga, L. F., Lepping, R. P.
core   +1 more source

Solar wind disturbances in th outer heliosphere caused by successive solar flares from the same active region [PDF]

, 1983
Solar wind disturbances caused by successive flares from the same active region are traced to about 20 AU, using the modeling method developed by Hakamada and Akasofu (1982).
Akasofu, S. I., Hakamada, K.
core   +1 more source

Modeling enstatite chondrites: Reduced rocks with a pinch of oxidized material (affected by varying H2O(g)) derived from planetesimals shocked during the epoch of giant–planet migration

Meteoritics &Planetary Science, Volume 61, Issue 1, Page 122-139, January 2026.
Abstract The O‐, N‐, Mo‐, Ru‐, Os‐, Cr‐, Ti‐, Ni‐, Fe‐, Nd‐, Ca‐, Zn‐, Sr‐, and Mg‐isotopic compositions of enstatite chondrites are essentially identical to those of the Earth and Moon. These correspondences suggest enstatite chondrites formed at ≈1 AU as the only known chondrite groups that accreted in the vicinity of a major planet. Bulk Earth has a
Alan E. Rubin
wiley   +1 more source

The extended coronal magnetic field [PDF]

Coronal magnetic field structure from photosphere to interplanetary ...
Wilcox, J. M.
core   +1 more source

Interplanetary magnetic field orientation and the magnetospheres of close-in exoplanets [PDF]

, 2010
E. P. G. Johansson, Mueller Joachim, U. Motschmann   +2 more
openalex   +1 more source

Magnetotail changes in relation to the solar wind magnetic field and magnetospheric substorms [PDF]

An attempt is made to understand some of the magnetotail dynamics by using simultaneous observations from several satellites: Explorers 33 and 35 in the solar wind, IMP 4 in the near magnetotail (30 RE), ATS 1, and OGO 5 in the magnetosphere.
Aubry, M. P., Mcpherron, R. L.
core   +1 more source