Sarsembayeva
A.T.,1 Sarsembay A.T.2
1Satbayev University,
Almaty, Kazakhstan
2School-Lyceum №250 named after T.Komekbayev,
Karmakchi area, Kyzylorda region, Kazakhstan
Development
of a new solar data visualisation tool
Solar
observatories are providing the world-wide community with a wealth of data,
covering wide time ranges (e.g. Solar and Heliospheric
Observatory, SOHO), multiple viewpoints (Solar TErrestrial
RElations Observatory, STEREO), and returning large amounts
of data (Solar Dynamics Observatory, SDO). In particular, the large volume of
SDO staggering volumes of data are accessible only from a few repositories, and
full-disk, full-cadence data for reasonable durations of scientific interest
are difficult to download, due to their size.
To address these challenges, we have started to develop a new solar data
visualisation tool using the Java programming language for a standalone
application type (GUI) [1]. A main page of the solar data visualisation tool is
shown in Fig.1.
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Figure 1: Main user interface |
References:
1.
Sarsembayeva A.T., Sarsembay A.T. Active processes in the Sun's atmosphere.
NEWS of the NAS RK. Series of Physical and Mathematical. №2 (294) (March-April), 2014г. P.214-218.