output
20062026
most citedSolar Coronal Jets: Observations, Theory, and Modeling

361 citations

Showing 2020 · physics.space-phShow all

8 papers · 2 filters

physics.space-ph2020★ 8 cited

Radiation Belt Response to Fast Reverse Shock at Geosynchronous Orbit

Ankush Bhaskar, David Sibeck, Shrikanth G. Kanekal +5

Fast reverse shocks (FRSs) cause the magnetosphere to expand, by contrast to the well-known compressions caused by the impact of fast forward shocks (FFS). Usually, FFSs are more g…

physics.space-ph2020★ 23 cited

Properties of the Sheath Regions of Coronal Mass Ejections with or without Shocks from STEREO in situ Observations near 1 AU

T. M. Salman, N. Lugaz, C. J. Farrugia +3

We examine 188 coronal mass ejections (CMEs) measured by the twin STEREO spacecraft during 2007-2016 to investigate the generic features of the CME sheath and the magnetic ejecta (…

physics.space-ph2020★ 16 cited

Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles

Rohit Chhiber, David Ruffolo, William H. Matthaeus +4

The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial transport and diffusion of charge…

physics.space-ph2020★ 11 cited

The Electron Proton Helium INstrument as an Example for a Space Weather Radiation Instrument

Patrick Kühl, Bernd Heber, Raúl Gómez-Herrero +3

The near-Earth energetic particle environment has been monitored since the 1970's. With the increasing importance of quantifying the radiation risk for, e.g. for the human explorat…

physics.space-ph2020★ 13 cited

The Extreme Space Weather Event in February/March 1941

Hisashi Hayakawa, Sean P. Blake, Ankush Bhaskar +3

Given the infrequency of extreme geomagnetic storms, it is significant to note the concentration of three extreme geomagnetic storms in 1941, whose intensities ranked fourth, twelf…

physics.space-ph2020★ 126 cited

Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone

D. Ruffolo, W. H. Matthaeus, R. Chhiber +11

Motivated by prior remote observations of a transition from striated solar coronal structures to more isotropic ``flocculated'' fluctuations, we propose that the dynamics of the in…