Neutrino astronomy with high spatial resolution is already existing

被引:0
|
作者
Rantsev-Kartinov, V. A. [1 ]
机构
[1] RRC Kurchatov Inst, Moscow 123182, Russia
关键词
D O I
10.1109/PPPS.2007.4652492
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
By basing on observations of skeletal structures of the Sun and assuming that some of them are located inside of star, and also that a filamentary (linear) matter (whose a model earlier was put forward by B.U. Rodionov) is in basis of these internal structures the author consider possible processes of images formation of these structures inside the Sun and theirs coming out into space and also gives an elementary estimations of its parameters, which allow: i) to form their images in a flux of electronic neutrinos; ii) to carry out these images from within of the Sun into space; iii) to develop these images in form of a concomitant flux of soft x-ray, which next is recorded by telescope of soft x-ray. It is supposed the processes considered here, actually, can be accepted as future base of neutrino astronomy with high spatial resolution.
引用
收藏
页码:1589 / 1594
页数:6
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