Radiative Effects in the Modelling of Accretion onto Stellar Magnetospheres

Author(s):  
Nikolai Pogorelov ◽  
Igor Kryukov ◽  
Ulrich Anzer ◽  
Guennadii Bisnovatyi-Kogan ◽  
Gerhard Börner
2003 ◽  
Vol 402 (1) ◽  
pp. 13-28 ◽  
Author(s):  
I. A. Kryukov ◽  
N. V. Pogorelov ◽  
U. Anzer ◽  
G. S. Bisnovatyi-Kogan ◽  
G. Börner

Tellus B ◽  
2009 ◽  
Vol 61 (1) ◽  
Author(s):  
Sebastian Otto ◽  
Eike Bierwirth ◽  
Bernadett Weinzierl ◽  
Konrad Kandler ◽  
Michael Esselborn ◽  
...  

2012 ◽  
Vol 5 (3) ◽  
pp. 176-183 ◽  
Author(s):  
Ali J. Chamkha ◽  
Mohamed Modather ◽  
Saber M.M. EL-Kabeir ◽  
Ahmed M. Rashad

1997 ◽  
Vol 182 ◽  
pp. 391-405 ◽  
Author(s):  
Lee Hartmann

Outflows from low-mass young stellar objects are thought to draw upon the energy released by accretion onto T Tauri stars. I briefly summarize the evidence for this accretion and outline present estimates of mass accretion rates. Young stars show a very large range of accretion rates, and this has important implications for both mass ejection and for the structure of stellar magnetospheres which may truncate T Tauri disks.


2021 ◽  
Vol 247 ◽  
pp. 118201
Author(s):  
Hao Wu ◽  
Tijian Wang ◽  
Qin'geng Wang ◽  
Yang Cao ◽  
Yawei Qu ◽  
...  

2011 ◽  
Vol 11 (12) ◽  
pp. 6049-6062 ◽  
Author(s):  
X. Yue ◽  
H. Liao ◽  
H. J. Wang ◽  
S. L. Li ◽  
J. P. Tang

Abstract. Mineral dust aerosol can be transported over the nearby oceans and influence the energy balance at the sea surface. The role of dust-induced sea surface temperature (SST) responses in simulations of the climatic effect of dust is examined by using a general circulation model with online simulation of mineral dust and a coupled mixed-layer ocean model. Both the longwave and shortwave radiative effects of mineral dust aerosol are considered in climate simulations. The SST responses are found to be very influential on simulated dust-induced climate change, especially when climate simulations consider the two-way dust-climate coupling to account for the feedbacks. With prescribed SSTs and dust concentrations, we obtain an increase of 0.02 K in the global and annual mean surface air temperature (SAT) in response to dust radiative effects. In contrast, when SSTs are allowed to respond to radiative forcing of dust in the presence of the dust cycle-climate interactions, we obtain a global and annual mean cooling of 0.09 K in SAT by dust. The extra cooling simulated with the SST responses can be attributed to the following two factors: (1) The negative net (shortwave plus longwave) radiative forcing of dust at the surface reduces SST, which decreases latent heat fluxes and upward transport of water vapor, resulting in less warming in the atmosphere; (2) The positive feedback between SST responses and dust cycle. The dust-induced reductions in SST lead to reductions in precipitation (or wet deposition of dust) and hence increase the global burden of small dust particles. These small particles have strong scattering effects, which enhance the dust cooling at the surface and further reduce SSTs.


2013 ◽  
Author(s):  
Guoyong Wen ◽  
Alexander Marshak ◽  
Lorraine Remer ◽  
Robert Levy ◽  
Norman Loeb ◽  
...  

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