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Space solar research: achievements and prospects


Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Kaluzhskoe shosse 4, Troitsk, Москва, 108840, Russian Federation

Space-based solar observations continue to provide new insights into the structure and dynamics of the Sun's interior and atmosphere. This paper uses helioseismic and magnetic data from the Helioseismic and Magnetic Imager of the Solar Dynamic Observatory (SDO) to present results on the Sun's subphotospheric and meridional flows and on the simulation of the solar dynamo and of the solar magnetic field variation. High spatial resolution observations of the solar atmosphere with SOHO, Hinode, SDO, IRIS, Hi-C, EUNIS, etc. provide detailed clues about the dynamics and fine structure of magnetic fields, flare energy release, and coronal mass ejections. Space projects with a promise to solve current solar physics problems are briefly reviewed.

Fulltext pdf (899 KB)
Fulltext is also available at DOI: 10.3367/UFNe.0185.201506k.0664
Keywords: Sun, space research, magnetic fields, dynamo, flares, mass ejections
PACS: 07.87.+v, 96.60.−j (all)
DOI: 10.3367/UFNe.0185.201506k.0664
URL: https://ufn.ru/en/articles/2015/6/j/
000361014200010
2015PhyU...58..621K
Citation: Kuznetsov V D "Space solar research: achievements and prospects" Phys. Usp. 58 621–629 (2015)
BibTexBibNote ® (generic)BibNote ® (RIS) MedlineRefWorks
PT Journal Article
TI Space solar research: achievements and prospects
AU Kuznetsov V D
FAU Kuznetsov VD
DP 10 Jun, 2015
TA Phys. Usp.
VI 58
IP 6
PG 621-629
RX 10.3367/UFNe.0185.201506k.0664
URL https://ufn.ru/en/articles/2015/6/j/
SO Phys. Usp. 2015 Jun 10;58(6):621-629

Received: 18th, April 2015, 25th, February 2015

Оригинал: Кузнецов В Д «Достижения и перспективы космических исследований Солнца» УФН 185 664–672 (2015); DOI: 10.3367/UFNr.0185.201506k.0664

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