Solar Rotation Velocity Determined by Coronal Bright Points – New Data and Analysis

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Solar Rotation Velocity Determined by Coronal Bright Points – New Data and Analysis. / Mulec, M.; Brajsa, Roman; Wöhl, Hubertus et al.
In: Central European astrophysical bulletin, Vol. 31, No. 1, 2007, p. 1-10.

Research output: Journal contributionsJournal articlesResearchpeer-review

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Mulec M, Brajsa R, Wöhl H, Hanslmeier A, Vrsnak B, Ruzdjak V et al. Solar Rotation Velocity Determined by Coronal Bright Points – New Data and Analysis. Central European astrophysical bulletin. 2007;31(1):1-10.

Bibtex

@article{a63745b8336d4676b5dd9482881807ed,
title = "Solar Rotation Velocity Determined by Coronal Bright Points – New Data and Analysis",
abstract = "Full-disc solar images obtained with the Extreme Ultraviolet Imaging Telescope on board the Solar and Heliospheric Observatory were used to analyse solar differential rotation determined by tracing coronal bright points. Rotation velocity residuals, meridional motions and their relationship are investigated for a new data set from October 1, 1999 to March 31, 2000. Further we take care for the evolution of the single structures, dividing them into Point-Like-Structures, Small Loops and Small Active Regions and analysing their variation in intensity and size.",
keywords = "Mathematics, Solar physics, solar rotation",
author = "M. Mulec and Roman Brajsa and Hubertus W{\"o}hl and Arnold Hanslmeier and Bojan Vrsnak and V. Ruzdjak and Jean-Francois Hochedez and John-Oliver Engler",
year = "2007",
language = "English",
volume = "31",
pages = "1--10",
journal = "Central European astrophysical bulletin",
issn = "1845-8319",
publisher = "University of Zagreb",
number = "1",

}

RIS

TY - JOUR

T1 - Solar Rotation Velocity Determined by Coronal Bright Points – New Data and Analysis

AU - Mulec, M.

AU - Brajsa, Roman

AU - Wöhl, Hubertus

AU - Hanslmeier, Arnold

AU - Vrsnak, Bojan

AU - Ruzdjak, V.

AU - Hochedez, Jean-Francois

AU - Engler, John-Oliver

PY - 2007

Y1 - 2007

N2 - Full-disc solar images obtained with the Extreme Ultraviolet Imaging Telescope on board the Solar and Heliospheric Observatory were used to analyse solar differential rotation determined by tracing coronal bright points. Rotation velocity residuals, meridional motions and their relationship are investigated for a new data set from October 1, 1999 to March 31, 2000. Further we take care for the evolution of the single structures, dividing them into Point-Like-Structures, Small Loops and Small Active Regions and analysing their variation in intensity and size.

AB - Full-disc solar images obtained with the Extreme Ultraviolet Imaging Telescope on board the Solar and Heliospheric Observatory were used to analyse solar differential rotation determined by tracing coronal bright points. Rotation velocity residuals, meridional motions and their relationship are investigated for a new data set from October 1, 1999 to March 31, 2000. Further we take care for the evolution of the single structures, dividing them into Point-Like-Structures, Small Loops and Small Active Regions and analysing their variation in intensity and size.

KW - Mathematics

KW - Solar physics

KW - solar rotation

M3 - Journal articles

VL - 31

SP - 1

EP - 10

JO - Central European astrophysical bulletin

JF - Central European astrophysical bulletin

SN - 1845-8319

IS - 1

ER -

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