Results 41 to 50 of about 2,118 (212)

Additional acceleration of solar-wind particles in current sheets of the heliosphere [PDF]

, 2015
Particles of fast solar wind in the vicinity of the heliospheric current sheet (HCS) or in a front of interplanetary coronal mass ejections (ICMEs) often reveal very peculiar energy or velocity profiles, density distributions with double or triple peaks,
V. Zharkova, Khabarova, Olga, V. Zharkova, O. Khabarova, Zharkova, Valentina   +4 more
core   +1 more source

Using a Heliospheric Upwinding eXtrapolation Technique to Magnetically Connect Different Regions of the Heliosphere

Frontiers in Physics, 2021
Understanding how coronal structure propagates and evolves from the Sun and into the heliosphere has been thoroughly explored using sophisticated MHD models.
Pete Riley, Opal Issan
doaj   +1 more source

Simultaneous interplanetary scintillation and Heliospheric Imager observations of a coronal mass ejection [PDF]

, 2008
We describe simultaneous Interplanetary Scintillation (IPS) and STEREO Heliospheric Imager (HI) observations of a coronal mass ejection (CME) on 16 May 2007. Strong CME signatures were present throughout the IPS observation.
Rouillard AP, Fallows, R. A., Rouillard, Alexis, Dorrian, G. D., Davies, J.A., Dorrian GD, Rouillard, A.P., Brown DS, Rouillard, A. P., Breen, A. R., Brown, D.S., Brown, Daniel, Fallows, R.A., Davies, Jackie, Breen, Andy, Fallows RA, Davies, J. A., Brown, Daniel Stephen, Davies JA, Dorrian, G.D., Fallows, Richard, Breen AR, Breen, A.R., Dorrian, Gareth   +23 more
core   +1 more source

Rotational Quasi-Periodicities and the Sun – Heliosphere Connection [PDF]

Solar Physics, 2008
Mutual quasi-periodicities near the solar-rotation period appear in time series based on the Earth's magnetic field, the interplanetary magnetic field, and signed solar-magnetic fields. Dominant among these is one at 27.03 +/- 0.02 days that has been highlighted by Neugebauer, et al. 2000, J. Geophys. Res., 105, 2315.
Lawrence, J. K., Cadavid, A. C., Ruzmaikin, A.   +2 more
openaire   +2 more sources

Analytical Model Nonequilibrium Inhomogeneous Plasma of the Heliosphere

, 2021
We prove that a nonequilibrium inhomogeneous giant gas discharge is realized in the heliosphere with huge values of the parameter E/N, which determines the temperature of electrons.
Philipp Vysikaylo (11794082)
core   +1 more source

Division II: The Sun and Heliosphere: (Le Soleil et Heliosphere) [PDF]

Transactions of the International Astronomical Union, 2000
Division II consists of Commissions 10 (Solar Activity), 12 (Solar Radiation and Structure), and 49 (Interplanetary Plasma and Heliosphere). More detailed information on IAU activities in each of these three areas can be found in the individual reports of the respective Commissions.The Division II OC briefly considered changes to the structure of our ...
Peter Foukal, Guoxiang Ai, Arnold Benz, Oddbjorn Engvold, Sami Solanki, Marek Vandas, Frank Verheest   +6 more
openaire   +1 more source

The International Heliophysical Year

Data Science Journal, 2009
The International Geophysical Year (IGY) of 1957, a broad-based and all-encompassing effort to push the frontiers of geophysics, resulted in a tremendous increase of knowledge in space physics, Sun-Earth Connection, planetary science and the heliosphere ...
Joseph M Davila, Barbara J Thompson, Nat Gopalswamy   +2 more
doaj   +1 more source

Fifty years of studying the GCR intensity during inversion of the heliospheric magnetic fields. II. HMF inversion on the inner heliospheric boundary

Solar-Terrestrial Physics
Phenomena in the outer layer of the solar atmosphere, the heliosphere, including the supersonic solar wind, the heliospheric magnetic field (HMF) carried by it, and cosmic rays propagating in the heliosphere are important for many processes occurring in ...
Krainev M. B., Kalinin M. S.
doaj   +1 more source

Corotating interaction regions as seen by the STEREO Heliospheric Imagers 2007 – 2010

, 2015
T.M. Conlon and A.O. Williams were supported by an STFC, UK studentship and S.E. Milan was supported by STFC grant ST/K001000/1. Date of Acceptance: 08/08/2015NASA’s Solar Terrestrial Relations Observatory (STEREO) mission has coincided with a pronounced
J. A. Davies, Conlon, Thomas Michael, Davies, J.A., Milan, S.E., S. E. Milan, T. M. Conlon, A. O. Williams, Williams, A.O.   +7 more
core   +1 more source

Solar wind stream interaction regions throughout the heliosphere

Living Reviews in Solar Physics, 2018
This paper focuses on the interactions between the fast solar wind from coronal holes and the intervening slower solar wind, leading to the creation of stream interaction regions that corotate with the Sun and may persist for many solar rotations. Stream
Ian G. Richardson
doaj   +1 more source