Results 101 to 110 of about 25,490 (221)

Suprathermal particle addition to solar wind pressure: possible influence on magnetospheric transmissivity of low energy cosmic rays?

, 2013
Energetic (suprathermal) solar particles, accelerated in the interplanetary medium, contribute to the solar wind pressure, in particular during high solar activity periods.
Bobik, P., Boschini, M. J., Consolandi, C., Della Torre, S., Gervasi, M., Grandi, D., Kudela, K., La Vacca, G., Mallamaci, M., Pensotti, S., Rancoita, P. G., Rozza, D., Tacconi, M.   +12 more
core  

Helmet and active streamers from radio observations [PDF]

Large coronal regions disconnected from any calcium plages and identified by their thermal emission at 169 mHz play a basic role in the sector structure of the interplanetary medium.
Avignon, Y., Axisa, F., Martres, M. J., Pick, M., Simon, P.   +4 more
core   +1 more source

Microstructure of the Interplanetary Medium [PDF]

High time resolution measurements of the interplanetary magnetic field and plasma reveal a complex microstructure which includes hydromagnetic wave and discontinuities.
Burlaga, L. F.
core   +1 more source

Solar-terrestrial response to large extension or long-duration solar gamma ray events [PDF]

Geofísica Internacional, 2000
Gamma ray lines (GRL) from the large event of 29 September 1989 were observed from a site about 25 degrees from the flare site. In June 1991, at least three long-duration GRL events were observed by several spacecraft.
A. Méndez Berhondo, R. E. Rodríguez Taboada, L. Miroshnichenko, R. Pérez Enríquez   +3 more
doaj  

Observational signatures of planetary tidal disruption events around solar-mass stars

Astronomy & Astrophysics
Context. The tidal disruption of planets by their host stars represents a growing area of interest in transient astronomy, offering insights into the final stages of planetary system evolution and the scattering of planets in gas-poor environments. Aims.
Montesinos Matías, Nayakshin Sergei, Elbakyan Vardan, Guo Zhen, Sucerquia Mario, Bayo Amelia, Zhu Zhaohuan   +6 more
doaj   +1 more source

Damping of high frequency waves in the solar wind [PDF]

Cyclotron damping by suprathermal fluxes of protons and electrons in the interplanetary medium will greatly attenuate high frequency Alfven waves and whistler waves within distances 1 AU of the sun.
Fisk, L. A., Goldstein, M. L.
core   +1 more source

Anomalous cosmic rays within the inner heliosphere: Observations of helium by the High Energy Telescope on board Solar Orbiter

Astronomy & Astrophysics
Context. The radial gradients of cosmic rays are key parameters in studies of the transport of particles in space. Solar Orbiter, launched on 2020 February 10, approaches the Sun approximately every half-a-year, with its closest perihelion distance of 0 ...
Xu Zigong, Wimmer-Schweingruber Robert F., Berger Lars, Kühl Patrick, Kollhoff Alexander, Heber Bernd, Böttcher Stephan I., Yang Liu, Heidrich-Meisner Verena, Strauss Roelf Du Toit, Gomez-Herrero Raúl, Rodriguez-Pacheco Javier, Pacheco Daniel, Leske Richard A.   +13 more
doaj   +1 more source

Identification and prediction of prolonged intervals of geomagnetic calm [PDF]

Geofísica Internacional, 2002
From the daily index Ap of geomagnetic activity, sequences of consecutive occurrence of Ap≤4 for four days and Ap≤7 for 8 days are identified in the period 1963-1998.
L.M. Barreto, G. K. Rangarajan
doaj  

Interplanetary stream interfaces [PDF]

At l AU there is a distinct boundary (the stream interface) at the leading edge of a stream in the solar wind, characterized by an abrupt drop in density, a similar increase in temperature and a small increase in speed.
Burlaga, L. F.
core   +1 more source

Preconditioning of the Interplanetary Medium Due To Isolated ICMEs

Journal of Geophysical Research: Space Physics
AbstractWe perform a systematic study of the preconditioning of the interplanetary (IP) medium due to isolated IP coronal mass ejections (ICMEs). Preconditioning is highly relevant when ICMEs, ejected in close succession and direction, modify the IP medium to allow subsequent ICMEs to propagate more freely, decelerate less, and retain higher kinetic ...
Primož Kajdič, Manuela Temmer, Xochitl Blanco‐Cano   +2 more
openaire   +2 more sources