Results 161 to 170 of about 278,597 (210)

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

Space Sci Rev
Nakamura R, Burch JL, Birn J, Chen LJ, Graham DB, Guo F, Hwang KJ, Ji H, Khotyaintsev YV, Liu YH, Oka M, Payne D, Sitnov MI, Swisdak M, Zenitani S, Drake JF, Fuselier SA, Genestreti KJ, Gershman DJ, Hasegawa H, Hoshino M, Norgren C, Shay MA, Shuster JR, Stawarz JE.   +24 more
europepmc   +1 more source

Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information. [PDF]

Sol Phys
Heinemann SG, Yang D, Jones SI, Pomoell J, Asvestari E, Henney CJ, Arge CN, Gizon L.   +7 more
europepmc   +1 more source

OpticalTrust: A Sensor-to-Blockchain Framework Using Free-Space Optical Communication. [PDF]

Sensors (Basel)
Bajaj P, Kataria A, Puri V, Gupta S, Min H.   +4 more
europepmc   +1 more source

Simulation Models for Exploring Magnetic Reconnection. [PDF]

Space Sci Rev
Shay M, Adhikari S, Beesho N, Birn J, Büchner J, Cassak P, Chen LJ, Chen Y, Cozzani G, Drake J, Guo F, Hesse M, Jain N, Pfau-Kempf Y, Lin Y, Liu YH, Oka M, Omelchenko Y, Palmroth M, Pezzi O, Reiff PH, Swisdak M, Toffoletto F, Toth G, Wolf RA.   +24 more
europepmc   +1 more source

Magnetic Reconnection in Space: An Introduction. [PDF]

Space Sci Rev
Burch JL, Nakamura R.
europepmc   +1 more source

Beyond Fiber: Toward Terahertz Bandwidth in Free-Space Optical Communication. [PDF]

Sensors (Basel)
Ullah R, Ullah S, Ren J, Alwageed HS, Mao Y, Qi Z, Wang F, Khan SA, Farooq U.   +8 more
europepmc   +1 more source

Study of micro-turbulence in the solar wind observed with interplanetary scintillation

, 1998
openaire   +1 more source

Shock waves propagation in the turbulent interplanetary plasma [PDF]

Astrophysics and Space Science, 1996
AbstractEffect of turbulence on interplanetary shock waves propagation is considered. It is shown that background turbulence results in the additional shock wave deceleration which may be comparable with the deceleration due to plasma sweeping. The turbulent deceleration is connected with the energy losses due to the strong turbulence amplification ...
Igor Chashei, V I Shishov
exaly   +3 more sources

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Turbulence properties associated with interplanetary shock waves

AIP Conference Proceedings, 2012
We calculate the power spectral densities of magnetic field fluctuations associated with interplanetary shock waves, utilizing in-situ magnetic field measurements from spacecraft ACE and Wind at 1AU. We derive related quantities both upstream and downstream of a shock as a function of time/distance away from the shock passage.
Gary P. Zank, Qiang Hu
exaly   +2 more sources

Observations of Turbulence near Interplanetary Travelling Shocks

AIP Conference Proceedings, 2005
The observations on magnetic field fluctuations and suprathermal ion spectra near the shocks driven by the coronal mass ejections during the time periods of the Bastille Day 2000 event and the Halloween 2003 events are summarized.
Martin Hilchenbach, R Kallenbach
exaly   +4 more sources