# Neutrino Astronomy with High Spatial Resolution is Already Existing

## TL;DR

This paper proposes a novel method for high-resolution neutrino astronomy by analyzing skeletal structures within the Sun and their associated electromagnetic emissions, suggesting a new observational approach.

## Contribution

It introduces a model linking solar skeletal structures to neutrino imaging and proposes a method for high-resolution neutrino astronomy based on these structures.

## Key findings

- Feasibility of imaging internal solar structures via neutrinos.
- Potential for high spatial resolution in neutrino astronomy.
- Correlation between solar skeletal structures and soft X-ray emissions.

## Abstract

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.

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Source: https://tomesphere.com/paper/0704.1105