Zobrazeno 1 - 10
of 3 954
pro vyhledávání: '"solar maximum"'
Autor:
Mata, Sebastián Rojas1 sebastian.rojasmata@irf.se, Wieser, Gabriella Stenberg1, Futaana, Yoshifumi1, Bader, Alexander2, Persson, Moa3, Fedorov, Andrey3, Tielong Zhang4
Publikováno v:
Journal of Geophysical Research. Space Physics. Jan2022, Vol. 127 Issue 1, p1-13. 13p.
Autor:
Altrock, Richard C.1 altrock@nso.edu
Publikováno v:
Solar Physics. Feb2014, Vol. 289 Issue 2, p623-629. 7p.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Ramesh, K.1 kbramesh@iiap.res.in, Lakshmi, N.2
Publikováno v:
Solar Physics. Feb2012, Vol. 276 Issue 1/2, p395-406. 12p. 5 Graphs.
Publikováno v:
Journal of Geophysical Research. Space Physics. Aug2019, Vol. 124 Issue 8, p7062-7071. 10p.
Autor:
Yue, Jia1 jia.yue@hamptonu.edu, Jian, Yongxiao1, Wang, Wenbin2, Meier, R.R.3, Burns, Alan2, Qian, Liying2, Jones, M.4, Wu, Dong L.5, Mlynczak, Martin6
Publikováno v:
Journal of Geophysical Research. Space Physics. Apr2019, Vol. 124 Issue 4, p3067-3082. 16p.
Autor:
T. W. David, Bolarinwa Adekoya, Chizurumoke Michael, Sofiat Adekoya, Omolara Adenuga, Semiu Kareem, Hamid Oladunjoye, Abayomi Ajetunmobi, Oyindamola Williams, Damilola Ogundele
Publikováno v:
Journal of Nigerian Society of Physical Sciences, Vol 4, Iss 4 (2022)
Magnetic reconnection can be used for studying the geoeffective processes in the coupled Sun–Solar wind – Magnetosphere dynamics leading to geomagnetic disturbance. In this study, 1-hour resolution solar wind plasma parameters from OMNIweb were u
Externí odkaz:
https://doaj.org/article/79be9b43e51a4a67b2a1dfaccb8fa5fc
Publikováno v:
Remote Sensing, Vol 15, Iss 1, p 195 (2022)
The ionospheric total electron content (TEC) is susceptible to factors, such as solar and geomagnetic activities, resulting in the enhancement of its non-stationarity and nonlinear characteristics, which aggravate the impact on radio communications.
Externí odkaz:
https://doaj.org/article/dbe95b0b231a4501bd1a617db2d06df3
Autor:
Bocchialini, K.1 karine.bocchialini@ias.u-psud.fr, Grison, B.2, Menvielle, M.3,4, Chambodut, A.5, Cornilleau-Wehrlin, N.6,7, Fontaine, D.7, Marchaudon, A.8,9, Pick, M.6, Pitout, F.8,9, Schmieder, B.6, Régnier, S.10, Zouganelis, I.11
Publikováno v:
Solar Physics. May2018, Vol. 293 Issue 5, p1-1. 1p.