Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Institute for Quantum Optics and Quantum Information InnsbruckAT973 papers
- Universität InnsbruckAT944 papers
- Institute of High Energy PhysicsCN842 papers
- University of ViennaAT835 papers
- Centre National de la Recherche ScientifiqueFR824 papers
- Space Research InstituteRU796 papers
- European Organization for Nuclear ResearchCH470 papers
- ETH ZurichCH461 papers
- Korea UniversityKR441 papers
- National Taiwan UniversityTW436 papers
- Panjab UniversityIN432 papers
- Sungkyunkwan UniversityKR432 papers
15 papers · 2 filters
The Magnetic Field Geometry of Small Solar Wind Flux Ropes Inferred from their Twist Distribution
W. Yu, C. J. Farrugia, N. Lugaz +4
This work extends recent efforts on the force-free modeling of large flux rope-type structures (magnetic clouds, MCs) to much smaller spatial scales. We first select small flux rop…
Multiple satellite analysis of the Earth's thermosphere and interplanetary magnetic field variations due to ICME/CIR events during 2003-2015
Sandro Krauss, Manuela Temmer, Susanne Vennerstroem
We present a refined statistical analysis based on interplanetary coronal mass ejections as well as co-rotating interaction regions for the time period 2003-2015 to estimate the im…
On the applicability of Taylor's hypothesis in streaming magnetohydrodynamic turbulence
R. A. Treumann, W. Baumjohann, Yasuhito Narita
We examine the range of applicability of Taylor's hypothesis used in observations of magnetic turbulence in the solar wind. We do not refer to turbulence theory. We simply ask whet…
On the ion-inertial range density power spectra in solar wind turbulence
R. A. Treumann, W. Baumjohann, Yasuhito Narita
A model-independent first-principle first-order investigation of the shape of turbulent density-power spectra in the ion-inertial range of the solar wind at 1 AU is presented. De-m…
Forecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard
Pete Riley, Leila Mays, Jesse Andries +15
Accurate forecasting of the properties of coronal mass ejections as they approach Earth is now recognized as an important strategic objective for both NOAA and NASA. The time of ar…
Electron-Scale Dynamics of the Diffusion Region during Symmetric Magnetic Reconnection in Space
R. B. Torbert, J. L. Burch, T. D. Phan +46
Magnetic reconnection is an energy conversion process important in many astrophysical contexts including the Earth's magnetosphere, where the process can be investigated in-situ. H…
CME impact on comet 67P/Churyumov-Gerasimenko
Niklas J. T. Edberg, M. Alho, M. André +22
We present Rosetta observations from comet 67P/Churyumov-Gerasimenko during the impact of a coronal mass ejection (CME). The CME impacted on 5-6 Oct 2015, when Rosetta was about 80…
On the Role of Separatrix Instabilities in Heating the Reconnection Outflow Region
M. Hesse, C. Norgren, P. Tenfjord +10
A study of the role of microinstabilities at the reconnection separatrix can play in heating the electrons during the transition from inflow to outflow is being presented. We find…
How accurately can we measure the reconnection rate for the MMS diffusion region event of 2017-07-11?
Kevin J. Genestreti, Takuma Nakamura, Rumi Nakamura +8
We investigate the accuracy with which the reconnection electric field can be determined from in-situ plasma data. We study the magnetotail electron diffusion region observed…
The mirror mode: A "superconducting'' space plasma analogue
R. A. Treumann, W. Baumjohann
We examine the physics of the magnetic mirror mode in its final state of saturation, the thermodynamic equilibrium, to demonstrate that the mirror mode is the analogue of a superco…
Electron mirror branch: Observational evidence from "historical" AMPTE-IRM and Equator-S measurements
R. A. Treumann, W. Baumjohann
Based on now historical magnetic and plasma data and available wave spectra from the AMPTE-IRM spacecraft, and on as well historical Equator-S high-cadence magnetic field observati…
Sub-ionospheric AKR: A possible mechanism for its transport down from the topside generation region to the F layer and ground
R. A. Treumann, W. Baumjohann, J. LaBelle
Recent theoretical work shows that "electron exhausts", elongated regions of depleted electron density shown by PIC codes to be generated in collisionless reconnection, can in prin…
Correlation of ICME Magnetic Fields at Radially Aligned Spacecraft
S. W. Good, R. J. Forsyth, J. P. Eastwood +1
The B-field structures of two ICMEs each observed by a pair of spacecraft close to radial alignment have been analysed. The ICMEs were observed in situ by MESSENGER and STEREO-B in…
Assessing the time dependence of reconnection with Poynting's theorem: MMS observations
Kevin J. Genestreti, Paul A. Cassak, Ali Varsani +3
We investigate the time dependence of electromagnetic-field-to-plasma energy conversion in the electron diffusion region of asymmetric magnetic reconnection. To do so, we consider…
The Physical Foundation of the Reconnection Electric Field
M. Hesse, Y. -H. Liu, L. -J. Chen +8
We report on computer simulations and analytic theory to provide a self-consistent understanding of the role of the reconnection electric field, which extends substantially beyond…