A new Java-based application in solar physics

Solar-based flares are one of the most impressive energetic events in the solar atmosphere. Given their part of job in the solar corona's energy balance and their function playing important role in the space weather, numerous observations researched the release of energy and induction of solar...

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Main Authors: A. Sarsembayeva, F. Belisarova, M. Odsuren, A. Sarsembay
Format: Article
Language:English
Published: Al-Farabi Kazakh National University 2019-12-01
Series:Physical Sciences and Technology
Online Access:http://phst/index.php/journal/article/view/175
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author A. Sarsembayeva
F. Belisarova
M. Odsuren
A. Sarsembay
author_facet A. Sarsembayeva
F. Belisarova
M. Odsuren
A. Sarsembay
author_sort A. Sarsembayeva
collection DOAJ
description Solar-based flares are one of the most impressive energetic events in the solar atmosphere. Given their part of job in the solar corona's energy balance and their function playing important role in the space weather, numerous observations researched the release of energy and induction of solar flares, focusing on the solar active. National solar observatories are providing the overall network with a wealth of data, covering extensive time ranges (e.g. Solar and Heliospheric Observatory, SOHO), numerous perspectives (Solar Terrestrial Relations Observatory, STEREO), and returning a lot of information (Solar Dynamics Observatory, SDO). Specifically, the huge amount of SDO data are accessible only from a few repositories, such type of data as a full-cadence data or full-disk of scientific concern are hard to download, because of their size. To address these difficulties we have begun to build up a new solar application using the Java programming language for a stand-alone application type (GUI).
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spelling doaj.art-4563c5091ba847e2be3c333fbb17dd022023-10-30T13:11:00ZengAl-Farabi Kazakh National UniversityPhysical Sciences and Technology2409-61212019-12-0163-4A new Java-based application in solar physicsA. SarsembayevaF. BelisarovaM. OdsurenA. Sarsembay Solar-based flares are one of the most impressive energetic events in the solar atmosphere. Given their part of job in the solar corona's energy balance and their function playing important role in the space weather, numerous observations researched the release of energy and induction of solar flares, focusing on the solar active. National solar observatories are providing the overall network with a wealth of data, covering extensive time ranges (e.g. Solar and Heliospheric Observatory, SOHO), numerous perspectives (Solar Terrestrial Relations Observatory, STEREO), and returning a lot of information (Solar Dynamics Observatory, SDO). Specifically, the huge amount of SDO data are accessible only from a few repositories, such type of data as a full-cadence data or full-disk of scientific concern are hard to download, because of their size. To address these difficulties we have begun to build up a new solar application using the Java programming language for a stand-alone application type (GUI). http://phst/index.php/journal/article/view/175
spellingShingle A. Sarsembayeva
F. Belisarova
M. Odsuren
A. Sarsembay
A new Java-based application in solar physics
Physical Sciences and Technology
title A new Java-based application in solar physics
title_full A new Java-based application in solar physics
title_fullStr A new Java-based application in solar physics
title_full_unstemmed A new Java-based application in solar physics
title_short A new Java-based application in solar physics
title_sort new java based application in solar physics
url http://phst/index.php/journal/article/view/175
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