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Pregled bibliografske jedinice broj: 361508

Proper Motions of Coronal Bright Points


Brajša, Roman; Wöhl, Hubertus; Vršnak, Bojan; Ruždjak, Vladimir; Clette, Frederic; Hochedez, Jean-Francois; Verbanac, Giuliana; Skokić, Ivica; Hanslmeier, Arnold
Proper Motions of Coronal Bright Points // Central European astrophysical bulletin, 32 (2008), 165-190 (recenziran, članak, znanstveni)


CROSBI ID: 361508 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
Proper Motions of Coronal Bright Points

Autori
Brajša, Roman ; Wöhl, Hubertus ; Vršnak, Bojan ; Ruždjak, Vladimir ; Clette, Frederic ; Hochedez, Jean-Francois ; Verbanac, Giuliana ; Skokić, Ivica ; Hanslmeier, Arnold

Izvornik
Central European astrophysical bulletin (1845-8319) 32 (2008); 165-190

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
solar rotation ; coronal bright points ; SOHO-EIT

Sažetak
Full-field full-resolution solar images obtained by the Extreme Ultraviolet Imaging Telescope on board the Solar and Heliospheric Observatory are used to analyse proper motions, velocity distributions, lifetimes, and diffusion coefficient of coronal bright points. The results obtained by the interactive method for three tracer subtypes (point-like structures, small loops, and small active regions) of coronal bright points for the period 4 June 1998 to 22 May 1999 are presented and compared. Distributions of meridional velocities, residual azimuthal velocities and velocities of proper motions are presented for the three tracer subtypes. Lifetimes up to 54 hours are found for 98% of all observed coronal bright points. Small active regions last on the average longer than point-like structures and small loops. The correlation between the absolute velocity of proper motion and lifetime is investigated and the mean free path (in the range from 3000 km to 15000 km) and the diffusion coefficient (approximately 200 km2/s) of coronal bright points are estimated. Finally, characteristics of the random walk process associated to the motions of coronal bright points are discussed in the Appendix.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekti:
007-0000000-1364 - Fizikalni procesi u atmosferama Sunca i zvijezda
007-0000000-1362 - Eruptivni procesi u Sunčevoj atmosferi
119-1193086-1314 - Istraživanje geomagnetskog polja i nehomogenosti litosfere u području Hrvatske (Herak, Davorka, MZOS ) ( CroRIS)

Ustanove:
Geodetski fakultet, Zagreb,
Prirodoslovno-matematički fakultet, Zagreb

Citiraj ovu publikaciju:

Brajša, Roman; Wöhl, Hubertus; Vršnak, Bojan; Ruždjak, Vladimir; Clette, Frederic; Hochedez, Jean-Francois; Verbanac, Giuliana; Skokić, Ivica; Hanslmeier, Arnold
Proper Motions of Coronal Bright Points // Central European astrophysical bulletin, 32 (2008), 165-190 (recenziran, članak, znanstveni)
Brajša, R., Wöhl, H., Vršnak, B., Ruždjak, V., Clette, F., Hochedez, J., Verbanac, G., Skokić, I. & Hanslmeier, A. (2008) Proper Motions of Coronal Bright Points. Central European astrophysical bulletin, 32, 165-190.
@article{article, author = {Braj\v{s}a, Roman and W\"{o}hl, Hubertus and Vr\v{s}nak, Bojan and Ru\v{z}djak, Vladimir and Clette, Frederic and Hochedez, Jean-Francois and Verbanac, Giuliana and Skoki\'{c}, Ivica and Hanslmeier, Arnold}, year = {2008}, pages = {165-190}, keywords = {solar rotation, coronal bright points, SOHO-EIT}, journal = {Central European astrophysical bulletin}, volume = {32}, issn = {1845-8319}, title = {Proper Motions of Coronal Bright Points}, keyword = {solar rotation, coronal bright points, SOHO-EIT} }
@article{article, author = {Braj\v{s}a, Roman and W\"{o}hl, Hubertus and Vr\v{s}nak, Bojan and Ru\v{z}djak, Vladimir and Clette, Frederic and Hochedez, Jean-Francois and Verbanac, Giuliana and Skoki\'{c}, Ivica and Hanslmeier, Arnold}, year = {2008}, pages = {165-190}, keywords = {solar rotation, coronal bright points, SOHO-EIT}, journal = {Central European astrophysical bulletin}, volume = {32}, issn = {1845-8319}, title = {Proper Motions of Coronal Bright Points}, keyword = {solar rotation, coronal bright points, SOHO-EIT} }

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