Zobrazeno 1 - 10
of 306
pro vyhledávání: '"Kuzin, S. A."'
Autor:
Sylwester, J., Stęślicki, M., Bąkała, J., Płocieniak, S., Szaforz, Ż., Kowaliński, M., Ścisłowski, D., Podgórski, P., Mrozek, T., Barylak, J., Makowski, A., Siarkowski, M., Kordylewski, Z., Sylwester, B., Kuzin, S., Kirichenko, A., Pertsov, A., Bogachev, S.
We present a novel X-ray assembly of functionally related instrument blocks intended to measure solar flare and active region (AR) spectra from within the Russian instrument complex KORTES, to be mounted aboard the International Space Station (ISS).
Externí odkaz:
http://arxiv.org/abs/1903.06163
Publikováno v:
A. A. Reva et al 2017 ApJ 851 108
We study the coronal mass ejection (CME) with a complex acceleration profile. The event occurred on April 23, 2009. It had an impulsive acceleration phase, an impulsive deceleration phase, and a second impulsive acceleration phase. During its evoluti
Externí odkaz:
http://arxiv.org/abs/1712.06430
Publikováno v:
The Astrophysical Journal, 840:64, 2017 May 10
We analyse nonlinear evolution of torsional Alfv\'en waves in a straight magnetic flux tube filled in with a low-$\beta$ plasma, and surrounded with a plasma of lower density. Such magnetic tubes model, in particular, a segment of a coronal loop or a
Externí odkaz:
http://arxiv.org/abs/1705.02790
Publikováno v:
ApJ, 814, 135, 2015
Fast magnetoacoustic waves guided along the magnetic field by plasma non-uniformities, in particular coronal loops, fibrils and plumes, are known to be highly dispersive, which leads to the formation of quasi-periodic wave trains excited by a broadba
Externí odkaz:
http://arxiv.org/abs/1510.07908
Akademický článek
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Autor:
Regnier, S., Alexander, C. E., Walsh, R. W., Winebarger, A. R., Cirtain, J., Golub, L., Korreck, K. E., Mitchell, N., Platt, S., Weber, M., De Pontieu, B., Title, A., Kobayashi, K., Kuzin, S., DeForest, C. E.
Publikováno v:
ApJ, 2014, 784, 134
Observing the Sun at high time and spatial scales is a step towards understanding the finest and fundamental scales of heating events in the solar corona. The Hi-C instrument has provided the highest spatial and temporal resolution images of the sola
Externí odkaz:
http://arxiv.org/abs/1402.2457
Some of local sources of the slow solar wind can be associated with spectroscopically detected plasma outflows at edges of active regions accompanied with specific signatures in the inner corona. The EUV telescopes (e.g. SPIRIT/CORONAS-F, TESIS/CORON
Externí odkaz:
http://arxiv.org/abs/1203.6756
Autor:
Sylwester, J., Kowalinski, M., Gburek, S., Siarkowski, M., Kuzin, S., Farnik, F., Reale, F., Phillips, K. J. H., Bakala, J., Gryciuk, M., Podgorski, P., Sylwester, B.
The SphinX X-ray spectrophotometer on the CORONAS-PHOTON spacecraft measured soft X-ray emission in the 1-15 keV energy range during the deep solar minimum of 2009 with a sensitivity much greater than GOES. Several intervals are identified when the X
Externí odkaz:
http://arxiv.org/abs/1203.6809
Autor:
Kolbasnikov, N. G.1 (AUTHOR) nikolay.kolbasnikov@gmail.com, Kuzin, S. A.1 (AUTHOR), Teteryatnikov, V. S.1 (AUTHOR), Adigamov, R. R.2 (AUTHOR), Sakharov, M. S.2 (AUTHOR), Matveev, M. A.2 (AUTHOR)
Publikováno v:
Metal Science & Heat Treatment. Jul2022, Vol. 64 Issue 3/4, p137-145. 9p.
Autor:
Kolbasnikov, N. G.1 (AUTHOR) nikolay.kolbasnikov@gmail.com, Kuzin, S. A.1 (AUTHOR), Teteryatnikov, V. S.1 (AUTHOR), Zhukov, N. V.1 (AUTHOR), Adigamov, R. R.2 (AUTHOR), Sakharov, M. S.2 (AUTHOR), Matveev, M. A.2 (AUTHOR)
Publikováno v:
Metal Science & Heat Treatment. May2022, Vol. 64 Issue 1/2, p71-79. 9p.