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Pregled bibliografske jedinice broj: 110642

Structure and stability of prominences with helical structure

Vršnak, Bojan; Ruždjak, Vladimir; Brajša, Roman; Džubur, Adil
Structure and stability of prominences with helical structure // Solar physics, 116 (1988), 45-60 (međunarodna recenzija, članak, znanstveni)

CROSBI ID: 110642 Za ispravke kontaktirajte CROSBI podršku putem web obrasca

Naslov
Structure and stability of prominences with helical structure

Autori
Vršnak, Bojan ; Ruždjak, Vladimir ; Brajša, Roman ; Džubur, Adil

Izvornik
Solar physics (0038-0938) 116 (1988); 45-60

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

Ključne riječi
.

Sažetak
.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA

Profili:

Avatar Url Adil Džubur (autor)

Avatar Url Vladimir Ruždjak (autor)

Avatar Url Roman Brajša (autor)

Avatar Url Bojan Vršnak (autor)

Citiraj ovu publikaciju:

Vršnak, Bojan; Ruždjak, Vladimir; Brajša, Roman; Džubur, Adil
Structure and stability of prominences with helical structure // Solar physics, 116 (1988), 45-60 (međunarodna recenzija, članak, znanstveni)
Vršnak, B., Ruždjak, V., Brajša, R. & Džubur, A. (1988) Structure and stability of prominences with helical structure. Solar physics, 116, 45-60.
@article{article, author = {Vr\v{s}nak, Bojan and Ru\v{z}djak, Vladimir and Braj\v{s}a, Roman and D\v{z}ubur, Adil}, year = {1988}, pages = {45-60}, keywords = {.}, journal = {Solar physics}, volume = {116}, issn = {0038-0938}, title = {Structure and stability of prominences with helical structure}, keyword = {.} }
@article{article, author = {Vr\v{s}nak, Bojan and Ru\v{z}djak, Vladimir and Braj\v{s}a, Roman and D\v{z}ubur, Adil}, year = {1988}, pages = {45-60}, keywords = {.}, journal = {Solar physics}, volume = {116}, issn = {0038-0938}, title = {Structure and stability of prominences with helical structure}, keyword = {.} }

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • SCI-EXP, SSCI i/ili A&HCI

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