Results 81 to 90 of about 5,952,631 (141)

Earth-affecting solar transients: a review of progresses in solar cycle 24. [PDF]

Prog Earth Planet Sci, 2021
Zhang J, Temmer M, Gopalswamy N, Malandraki O, Nitta NV, Patsourakos S, Shen F, Vršnak B, Wang Y, Webb D, Desai MI, Dissauer K, Dresing N, Dumbović M, Feng X, Heinemann SG, Laurenza M, Lugaz N, Zhuang B.   +18 more
europepmc   +1 more source

Anisotropic Proton Heating by Kinetic Instabilities in Corotating Interaction Regions

The Astrophysical Journal
Corotating interaction regions (CIRs), formed by the interaction of fast and slow solar wind streams, are characterized by strong compression, enhanced turbulence, and elevated proton temperatures.
Kishor Kumbhar, Anil Raghav, Zubair Shaikh, Utkarsh Sharma, Mohit Shah, Omkar Dhamane, Ajay Kumar, Mariyam Karari, Shubham Kadam, Ankush Bhaskar, Kalpesh Ghag, S. Tulasiram   +11 more
doaj   +1 more source

Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium. [PDF]

Space Sci Rev, 2022
Rankin JS, Bindi V, Bykov AM, Cummings AC, Della Torre S, Florinski V, Heber B, Potgieter MS, Stone EC, Zhang M.   +9 more
europepmc   +1 more source

Variable Linear Polarization across Optical Emission Lines of the Wolf–Rayet Star EZ Canis Majoris and Its Relation to Corotating Interaction Regions

The Astrophysical Journal
Structure can be found on all scales in the winds of hot, luminous stars, including Wolf–Rayet (W-R) stars. Large-scale, spiral-shaped corotating interaction regions (CIRs) are thought to be present, causing quasi-periodic variability.
L. Fabiani, N. St-Louis, A. F. J. Moffat, A-N. Chené, R. Ignace   +4 more
doaj   +1 more source

Energetic particle acceleration at corotating interaction regions: Ulysses results [PDF]

, 1997
We present here statistical properties of energetic ions (tilde 1 MeV) accelerated by corotating interaction regions observed at the Ulysses spacecraft.
Gosling, J. T., Marsden, R. G., Balogh, A., Desai, M. I., Forsyth, R. J., Sanderson, T. R.   +5 more
core  

Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Revisited: In-Flight Calibrations, Lessons Learned and Scientific Advances. [PDF]

Space Sci Rev, 2023
Gkioulidou M, Mitchell DG, Manweiler JW, Lanzerotti LJ, Gerrard AJ, Ukhorskiy AY, Keika K, Mouikis CG, Kistler LM.   +8 more
europepmc   +1 more source

Corotating Interaction Regions and clumping

, 2008
We present hydrodynamical models for Corotating Interaction Regions, which were used by Lobel (2007) to model the Discrete Absorption Components in HD 64760.
Blomme, R.
core  

Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko. [PDF]

J Geophys Res Space Phys, 2023
Goetz C, Scharré L, Wedlund CS, Moeslinger A, Nilsson H, Odelstad E, Taylor MGGT, Volwerk M.   +7 more
europepmc   +1 more source

Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections. [PDF]

Space Sci Rev, 2021
Nitta NV, Mulligan T, Kilpua EKJ, Lynch BJ, Mierla M, O'Kane J, Pagano P, Palmerio E, Pomoell J, Richardson IR, Rodriguez L, Rouillard AP, Sinha S, Srivastava N, Talpeanu DC, Yardley SL, Zhukov AN.   +16 more
europepmc   +1 more source

Turning Instrument Background Into Science Data for Structural Features of Radiation Belts. [PDF]

J Geophys Res Space Phys, 2021
Ganushkina NY, Dandouras I, Liemohn MW, Rème H, Cao J.   +4 more
europepmc   +1 more source