Results 111 to 120 of about 5,692 (228)

Propagation of Interplanetary Disturbances in the Outer Heliosphere

, 2005
Contents include the following: 1. We have developed a one-dimensional, spherically symmetric, multi-fluid MHD model that includes solar wind protons and electrons, pickup ions, and interstellar neutral hydrogen.
Wang, Chi
core  

Transport of Solar Wind Fluctuations: A Two-Component Model

, 2011
We present a new model for the transport of solar wind fluctuations which treats them as two interacting incompressible components: quasi-two-dimensional turbulence and a wave-like piece.
Matthaeus, William H., P. A. Isenberg, Breech, B., Isenberg, P. A., Matthaeus, W. H., C. W. Smith, Smith, C. W., Oughton, Sean, S. Oughton, Smith, Charles W., W. H. Matthaeus, Oughton, S., B. Breech, Breech, Ben   +13 more
core   +1 more source

Galactic Cosmic Rays in the Outer Heliosphere

, 2010
We report a next generation model of galactic cosmic ray (GCR) transport in the three dimensional heliosphere. Our model is based on an accurate three-dimensional representation of the heliospheric interface.
Pogorelov, N. V., Florinski, V., Adams, J. H., Washimi, H.   +3 more
core  

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

Transactions of the International Astronomical Union, 2002
Arnold O. Benz, Thomas J. Bogdan, Peter V. Foukal, Donald B. Melrose, Sami K. Solanki, Marek Vandas, David F. Webb   +6 more
openaire   +1 more source

Modeling of electrons in the heliosphere

, 2016
PhD (Space Physics), North-West University, Potchefstroom Campus, 2016The propagation and modulation of electrons in the heliosphere play an important part in improving our understanding and assessment of the processes of solar modulation.
Nndanganeni, Rendani Rejoyce
core  

The Whole Heliosphere Interval: Campaign Summaries and Early Results

, 2008
The Whole Heliosphere Interval (WHI) is an internationally coordinated observing and modeling effort to characterize the 3-dimensional interconnected solar-heliospheric-planetary system - a.k.a. the "heliophysical" system.
Kozyra, Janet U., Thompson, Barbara J., Gibson, Sarah E.   +2 more
core  

Particles accelerated by shocks in the heliosphere

, 1988
The populations of energetic ions accelerated by shocks in the heliosphere are reviewed briefly.
Lee, Martin A.
core  

USING HELIOSPHERE LEARNING MEDIA TO MOTIVATE ELEMENTARY SCHOOL STUDENTS

This study aims to use heliosphere media to increase the learning motivation of SDN 3 Ketan\u27s grade VI science students. Sixteen students are the subjects of the classroom action research (CAR) methodology.
Aulia, Abinda Nova, Alfina Sukma, Putri Zudhah Ferryka, , dkk, Adinda Putri Sabila, Ainun Nadia   +4 more
core   +1 more source

Oblique Compressible Waves in the Reconnection Exhaust Region Embedded in the Inner Heliospheric Current Sheet Observed by Parker Solar Probe

The Astrophysical Journal
Magnetic reconnection is an important physical process of energy conversion in the heliosphere. Parker Solar Probe (PSP) passes through current sheets of the inner heliosphere and is likely to encounter magnetic reconnection events there. PSP traversed a
Rui Zhuo, Jiansen He, Die Duan, Xingyu Zhu, Chuanpeng Hou   +4 more
doaj   +1 more source

Exploration of heliosphere by interplanetary scintillation

, 1986
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory operating at a frequency of 103 MHz in western India for exploration of the heliosphere by the interplanetary scintillation (IPS) technique. The three radio
Vats, H. O., Sharma, A. K., Alurkar, S. K., Bhonsle, R. V., Degaonkar, S. S.   +4 more
core   +1 more source