Use my Search Websuite to scan PubMed, PMCentral, Journal Hosts and Journal Archives, FullText. Kick-your-searchterm to multiple Engines kick-your-query now !>

A dictionary by aggregated review articles of nephrology, medicine and the life sciences Your one-stop-run pathway from word to the immediate pdf of peer-reviewed on-topic knowledge.

10.1038/srep43147 http://scihub22266oqcxt.onion/10.1038/srep43147 C5335648!5335648!28256538     free     free     free Warning: file_get_contents(https://eutils.ncbi.nlm.nih.gov/entrez/eutils/elink.fcgi?dbfrom=pubmed&id=28256538&cmd=llinks): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 215 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Sci+Rep 2017 ; 7 (ä): ä Nephropedia Template TP {{tp|p=28256538|t=2017. High-frequency torsional Alfvén waves as an energy source for coronal heating |pdf=|usr=}}{{28256538}} gab.com Text High-frequency torsional Alfvén waves as an energy source for coronal heating JO: Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=28256538 #FOAvip The existence of the Sun?s hot atmosphere and the solar wind acceleration continues to be an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) modes and dissipation of magnetic energy contribute to heating and the mass cycle of the solar atmosphere, yet direct evidence of such processes often generates debate. Ground-based 1-m Swedish Solar Telescope (SST)/CRISP, H? 6562.8?Å observations reveal, for the first time, the ubiquitous presence of high frequency (~12?42?mHz) torsional motions in thin spicular-type structures in the chromosphere. We detect numerous oscillating flux tubes on 10 June 2014 between 07:17 UT to 08:08 UT in a quiet-Sun field-of-view of 60??×?60? (1??=?725?km). Stringent numerical model shows that these observations resemble torsional Alfvén waves associated with high frequency drivers which contain a huge amount of energy (~105?W?m?2) in the chromosphere. Even after partial reflection from the transition region, a significant amount of energy (~103?W?m?2) is transferred onto the overlying corona. We find that oscillating tubes serve as substantial sources of Alfvén wave generation that provide sufficient Poynting flux not only to heat the corona but also to originate the supersonic solar wind. Twit Text FOAVip High-frequency torsional Alfvén waves as an energy source for coronal heating ????Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=28256538 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28256538 #FOAvip English Wikipedia <ref>{{Cite pmid|28256538}}</ref> High-frequency torsional Alfvén waves as an energy source for coronal heating #MMPMID28256538 Srivastava AK; Shetye J; Murawski K; Doyle JG; Stangalini M; Scullion E; Ray T; Wójcik DP; Dwivedi BN Sci Rep 2017[]; 7 (ä): ä PMID28256538show ga The existence of the Sun?s hot atmosphere and the solar wind acceleration continues to be an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) modes and dissipation of magnetic energy contribute to heating and the mass cycle of the solar atmosphere, yet direct evidence of such processes often generates debate. Ground-based 1-m Swedish Solar Telescope (SST)/CRISP, H? 6562.8?Å observations reveal, for the first time, the ubiquitous presence of high frequency (~12?42?mHz) torsional motions in thin spicular-type structures in the chromosphere. We detect numerous oscillating flux tubes on 10 June 2014 between 07:17 UT to 08:08 UT in a quiet-Sun field-of-view of 60??×?60? (1??=?725?km). Stringent numerical model shows that these observations resemble torsional Alfvén waves associated with high frequency drivers which contain a huge amount of energy (~105?W?m?2) in the chromosphere. Even after partial reflection from the transition region, a significant amount of energy (~103?W?m?2) is transferred onto the overlying corona. We find that oscillating tubes serve as substantial sources of Alfvén wave generation that provide sufficient Poynting flux not only to heat the corona but also to originate the supersonic solar wind. äHigh-frequency torsional Alfvén waves as an energy source for coronal (epmc).pdf DeepDyve Pubget Overpricing