Results 11 to 20 of about 283,816 (315)

Properties of mass-loading shocks, 2. Magnetohydrodynamics [PDF]

open access: yes, 1992
The one-dimensional magnetohydrodynamics of shocked flows subjected to significant mass loading are considered. Recent observations at comets Giacobini-Zinner and Halley suggest that simple nonreacting MHD is an inappropriate description for active ...
Oughton, Sean   +3 more
core   +1 more source

Shock the heat shock network [PDF]

open access: yesJournal of Clinical Investigation, 2009
The targeting of tumors is made possible through establishing protein signatures specific for each cancer type. The recent recognition of the higher expression levels of HSP90 and its accumulation in tumor cell mitochondria has made the HSP90 network a feasible target for neutralization.
Cigdem, Atay   +2 more
openaire   +2 more sources

Probing Magnetic Fields and Acceleration Mechanisms in Blazar Jets with X-ray Polarimetry

open access: yesGalaxies, 2021
X-ray polarimetry promises us an unprecedented look at the structure of magnetic fields and on the processes at the base of acceleration of particles up to ultrarelativistic energies in relativistic jets.
Fabrizio Tavecchio
doaj   +1 more source

Do Bitcoin and Traditional Financial Assets Act as an Inflation Hedge during Stable and Turbulent Markets? Evidence from High Cryptocurrency Adoption Countries

open access: yesAxioms, 2022
This study analyzes whether Bitcoin, gold, oil, and stock have the ability to hedge against inflation in high cryptocurrency adoption countries in the periods from January 2010 to March 2021.
Panisara Phochanachan   +3 more
doaj   +1 more source

Stress on Real Income in Russian Regions Under the Pandemic and Sanctions [PDF]

open access: yesПространственная экономика, 2023
The study is devoted to assessing the stress of real incomes of the population (regarding wages) and the real financial result of enterprises in the Russian regions during the pandemic and sanctions shocks of 2017–2023.
Marina Yurievna Malkina
doaj   +1 more source

A Multi-Event Study of Early-Stage SEP Acceleration by CME-Driven Shocks—Sun to 1 AU

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The solar corona between below 10 solar radii is an important region for early acceleration and transport of solar energetic particles (SEPs) by coronal mass ejection-driven shock waves.
Kamen Kozarev   +4 more
doaj   +1 more source

Uncertainty Shocks are Aggregate Demand Shocks [PDF]

open access: yesFederal Reserve Bank of San Francisco, Working Paper Series, 2012
Abstract Search frictions in the labor market give rise to a new option-value channel through which uncertainty affects aggregate economic activity, and the effects of which are reinforced by the presence of nominal rigidities. With these features, an increase in uncertainty resembles an aggregate demand shock because it increases unemployment and ...
Sylvain Leduc, Zheng Liu
openaire   +3 more sources

The interplanetary causes of geomagnetic activity during the 7–17 March 2012 interval: a CAWSES II overview

open access: yesJournal of Space Weather and Space Climate, 2014
This overview paper presents/discusses the major solar, interplanetary, magnetospheric, and ionospheric features of the CAWSES II interval of study: 7–17 March 2012. Magnetic storms occurred on 7, 9, 12, and 15 March with peak SYM-H intensities of −98 nT,
Tsurutani Bruce T.   +7 more
doaj   +1 more source

Being Resilient in Challenging Times in Food Supply Chains

open access: yesEngineering Proceedings, 2023
Resilience has been described in many ways and in this paper is considered as the ability of an organization or wider food supply chain to not just ‘bounce back’ to a steady state, but to ‘bounce forward’ or ‘bounce without breaking’ to a new sense of ...
Louise Manning
doaj   +1 more source

Transient Foreshock Structures Upstream of Mars: Implications of the Small Martian Bow Shock

open access: yesGeophysical Research Letters, 2023
The typical subsolar stand‐off distance of Mars' bow shock is of the order of a solar wind ion convective gyroradius, making it highly non‐planar to incident ions.
H. Madanian   +13 more
doaj   +1 more source

Home - About - Disclaimer - Privacy