Edward P. Ney
http://dbpedia.org/resource/Edward_P._Ney an entity of type: Thing
إدوارد بي ني (بالإنجليزية: Edward P. Ney) هو فيزيائي أمريكي، ولد في 28 أكتوبر 1920 في منيابولس في الولايات المتحدة، وتوفي بنفس المكان في 9 يوليو 1996.
rdf:langString
Edward Purdy Ney (October 28, 1920 – July 9, 1996) was an American physicist who made major contributions to cosmic ray research, atmospheric physics, heliophysics, and infrared astronomy. He was a discoverer of cosmic ray heavy nuclei and of solar proton events. He pioneered the use of high-altitude balloons for scientific investigations and helped to develop procedures and equipment that underlie modern scientific ballooning. He was one of the first researchers to put experiments aboard spacecraft.
rdf:langString
rdf:langString
إدوارد بي ني
rdf:langString
Edward P. Ney
rdf:langString
Edward P. Ney
rdf:langString
Edward P. Ney
rdf:langString
Minneapolis, MN
xsd:date
1996-07-09
xsd:date
1920-10-28
xsd:integer
34322758
xsd:integer
1113998090
rdf:langString
University of MinnesotaUniversity of Virginia
xsd:date
1920-10-28
rdf:langString
Photo provided by Frank B. McDonald
xsd:date
1996-07-09
xsd:integer
220
rdf:langString
American
rdf:langString
إدوارد بي ني (بالإنجليزية: Edward P. Ney) هو فيزيائي أمريكي، ولد في 28 أكتوبر 1920 في منيابولس في الولايات المتحدة، وتوفي بنفس المكان في 9 يوليو 1996.
rdf:langString
Edward Purdy Ney (October 28, 1920 – July 9, 1996) was an American physicist who made major contributions to cosmic ray research, atmospheric physics, heliophysics, and infrared astronomy. He was a discoverer of cosmic ray heavy nuclei and of solar proton events. He pioneered the use of high-altitude balloons for scientific investigations and helped to develop procedures and equipment that underlie modern scientific ballooning. He was one of the first researchers to put experiments aboard spacecraft. In 1963, Ney became one of the first infrared astronomers. He founded O'Brien Observatory, where he and his colleagues discovered that certain stars are surrounded by grains of carbon and silicate minerals and established that these grains, from which planets are formed, are ubiquitous in circumstellar winds and regions of star formation.
xsd:nonNegativeInteger
66970
