Results 21 to 30 of about 833,845 (284)
Link between the chromospheric network and magnetic structures of the corona [PDF]
, 2006 Recent work suggested that the traditional picture of the corona above the quiet Sun being rooted in the magnetic concentrations of the chromospheric network alone is strongly questionable.
Beck +17 more
core +2 more sources
Frontiers in Neurology, 2020 Stroke survivors show greater postural oscillations and altered muscular activation compared to healthy controls. This results in difficulties in walking and standing, and in an increased risk of falls.
Alice De Luca +13 more
doaj +1 more source
Applied Sciences, 2021 In recent years, researchers in the pharmaceutical and food areas focused on finding the best ways to take advantage of functional ingredients present in jackfruit tissues and by-products such as phenolics and pectin.
Frida Camila Cruz-Casillas +2 more
doaj +1 more source
Warm and thick corona for magnetically supported disk in GBHB
, 2019 This paper is devoted to self-consistent modeling of the magnetically supported accretion disk with optically thick warm corona based on first principles. In our model, we consider the gas heating by magneto-rotational instability (MRI) dynamo.
Gronkiewicz, Dominik, Różańska, Agata
core +1 more source
CENP-F stabilizes kinetochore-microtubule attachments and limits dynein stripping of corona cargoes [PDF]
, 2020 Accurate chromosome segregation demands efficient capture of microtubules by kinetochores and their conversion to stable bioriented attachments that can congress and then segregate chromosomes.
Allan +80 more
core +1 more source
, 2012 We investigate the accretion process in high-luminosity AGNs (HLAGNs) in the scenario of the disk evaporation model. Based on this model, the thin disk can extend down to the innermost stable circular orbit (ISCO) at accretion rates higher than $0.02\dot{
Liu, B. F. +3 more
core +1 more source
Galactic fountains and the rotation of disc-galaxy coronae [PDF]
, 2011 In galaxies like the Milky Way, cold (~ 10^4 K) gas ejected from the disc by stellar activity (the so-called galactic-fountain gas) is expected to interact with the virial-temperature (~ 10^6 K) gas of the corona.
Anderson +43 more
core +3 more sources
Symposium - International Astronomical Union, 1997 The last two decades have seen the emergence of a new field in stellar astrophysics, the study of stellar coronae mostly in X-ray domain. With the advent of soft X-ray imagery X-ray emission was found from many thousands of solar-like stars. I will summarize the most important findings of X-ray surveys of late type stars and put the results in the ...
openaire +1 more source
Astrophysics and Space Science, 2007 9 pages, 6 figures; talk at "Isolated Neutron Stars: from the Interior to the Surface," London, April ...
Beloborodov, A. M., Thompson, C.
openaire +2 more sources