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10.12942/lrsp-2014-2 http://scihub22266oqcxt.onion/10.12942/lrsp-2014-2 C4841185!4841185 !27194956     free     free     free Warning: file_get_contents(https://eutils.ncbi.nlm.nih.gov/entrez/eutils/elink.fcgi?dbfrom=pubmed&id=27194956 &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 Warning: imagejpeg(C:\Inetpub\vhosts\kidney.de\httpdocs\phplern\27194956 .jpg): Failed to open stream: No such file or directory in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 117       Living+Rev+Sol+Phys 2014 ; 11 (ä): 2 Nephropedia Template TP {{tp|p=27194956 |t=2014. Infrared Solar Physics |pdf=|usr=}}{{27194956 }} gab.com Text Infrared Solar Physics JO: Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194956 #FOAvip The infrared solar spectrum contains a wealth of physical data about our Sun, and is explored using modern detectors and technology with new ground-based solar telescopes. The scientific motivation behind exploring these wavelengths is presented, along with a brief look at the rich history of observations here. Several avenues of solar physics research exploiting and benefiting from observations at infrared wavelengths from roughly 1000 nm to 12 400 nm are discussed, and the instrument and detector technology driving this research is briefly summarized. Finally, goals for future work at infrared wavelengths are presented in conjunction with ground and space-based observations. Twit Text FOAVip Infrared Solar Physics ????Living Rev Sol Phys http://www.kidney.de/pget.php?&tw=1&pmid=27194956 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27194956 #FOAvip English Wikipedia <ref>{{Cite pmid|27194956 }}</ref> Infrared Solar Physics #MMPMID27194956 Penn MJ Living Rev Sol Phys 2014[]; 11 (ä): 2 PMID27194956 show ga The infrared solar spectrum contains a wealth of physical data about our Sun, and is explored using modern detectors and technology with new ground-based solar telescopes. The scientific motivation behind exploring these wavelengths is presented, along with a brief look at the rich history of observations here. Several avenues of solar physics research exploiting and benefiting from observations at infrared wavelengths from roughly 1000 nm to 12 400 nm are discussed, and the instrument and detector technology driving this research is briefly summarized. Finally, goals for future work at infrared wavelengths are presented in conjunction with ground and space-based observations. äInfrared Solar Physics (epmc).pdf DeepDyve Pubget Overpricing