Zobrazeno 1 - 7
of 7
pro vyhledávání: '"K. I. Nikolskaya"'
Autor:
K. I. Nikolskaya, T. E. Valchuk
Publikováno v:
Astronomical & Astrophysical Transactions. 18:279-286
A concept of the solar corona and the solar wind resulting from the interaction between the solar primary high speed mass emanation and over-photospheric magnetic fields is outlined and developed. The model arises from the recent view of the solar co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::082156f363445da5784f58a24f963203
https://doi.org/10.1080/10556799908203067
https://doi.org/10.1080/10556799908203067
Autor:
K. I. Nikolskaya, M. A. Mogilevsky
Publikováno v:
The Sun: New Challenges ISBN: 9783642294167
We analyze, generalize, and interpret the data for the permanent solar wind (PSW) velocities measured on board of Ulysses (SWOOPS). A finding of a principal importance extracted from Ulysses’ observations is a discovery of the clear-cut inverse cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::64d003866e24c6decee6d5349f31a91f
https://doi.org/10.1007/978-3-642-29417-4_17
https://doi.org/10.1007/978-3-642-29417-4_17
Autor:
K. I. Nikolskaya, E. I. Mogilevsky
Publikováno v:
Proceedings of the International Astronomical Union. 2004:129-130
Solar magnetic field polarity reversal (SMFPR) happens every 10-11 years. However untill now there is no clear understanding in what way this process is carried out. Results represented here are a by-product of the coronal hole study based on taken f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::30ab30873817d5fa81f33d5126b2e480
https://doi.org/10.1017/s1743921304005381
https://doi.org/10.1017/s1743921304005381
Autor:
K. I. Nikolskaya
Publikováno v:
Mechanisms of Chromospheric and Coronal Heating ISBN: 9783642874574
Temperature inhomogeneities of the plasma in the active and undisturbed solar corona are investigated on the basis of ground eclipse observations of coronal spectra and monochromatic images. It is shown that the lower solar corona is a mixture of nea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e96c109b5580ce502cec83cf32c34a0b
https://doi.org/10.1007/978-3-642-87455-0_24
https://doi.org/10.1007/978-3-642-87455-0_24
Autor:
K. I. Nikolskaya
Publikováno v:
Solar Physics. 56:71-77
A series of 31 large scale spectra of the spicules near H8-Heζ lines λ 3889 A has been photographed at different heights (1500–5000 km) with 53-cm coronagraph. The solar image was 121 mm in diameter, dispersion and spatial resolution were respect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::12a638173dab02e4dd763e953c01e932
https://doi.org/10.1007/bf00152634
https://doi.org/10.1007/bf00152634
Publikováno v:
Solar Physics. 21:332-350
Slit spectrograms of a quiescent prominence and the inner corona (h⩽2.5 arc min) in the range λλ3400–7000 A (dispersion 6–10 A/mm) were obtained. From an analysis of the Stark effect on the Balmer lines (up to number 36) the electron density
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bf14257dcd9debd6abaa264c2cc27c74
https://doi.org/10.1007/bf00154285
https://doi.org/10.1007/bf00154285
Autor:
K. I. Nikolskaya, V. G. Utrobin
Publikováno v:
Solar Physics. 91
The physical properties in the coronal disturbance (CD) (W90, N25°) associated with an active prominence are investigated on the basis of the intensities and profiles of λ 5694 A Caxv and λ 6702 A Nixv lines and continuum measured in the eclipse c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::927dc7400b12d9b30bddc06eb5970d73
https://doi.org/10.1007/bf00213620
https://doi.org/10.1007/bf00213620