Zobrazeno 1 - 10
of 269
pro vyhledávání: '"H. S. Ahluwalia"'
Autor:
H. S. Ahluwalia
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:2559-2561
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0fa5a8797d027e20110128e0f89b7395
https://doi.org/10.1029/1998ja900073
https://doi.org/10.1029/1998ja900073
Autor:
Robert M. Wilson, David H. Hathaway
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:2555-2558
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f983638d5f5cc25517331e6f2806512a
https://doi.org/10.1029/1998ja900074
https://doi.org/10.1029/1998ja900074
Autor:
H. S. Ahluwalia, R. C. Ygbuhay
Publikováno v:
Advances in Astronomy, Vol 2012 (2012)
Ahluwalia and Jackiewicz (2011) have predicted that sunspot cycle 24 will be only half as active as cycle 23, reaching its peak in May 2013±6 months. Here, we discuss the timeline for cycle 24 since its onset in December, 2008 and compare it to the
Externí odkaz:
https://doaj.org/article/21231fb1607840909d1f24feacd17f50
Autor:
Wilson, Robert M., Hathaway, David H.
Publikováno v:
Journal of Geophysical Research. Space Physics; 1999, Vol. 104 Issue A2, p2555-2558, 4p
Autor:
R. C. Ygbuhay, H. S. Ahluwalia
Publikováno v:
Solar Physics. 291:3807-3815
Recently Clette et al. (Space Sci. Rev. 186, 35, 2014) completed the first revision of the international sunspot number SSN(V2) since its creation by Wolf in 1849 SSN(V1) starting in 1700 and ending in May 2015. The yearly values of SSN(V2) are large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e38033d284726fce15c195dfe680f0d1
https://doi.org/10.1007/s11207-016-0996-9
https://doi.org/10.1007/s11207-016-0996-9
Autor:
Ahluwalia, H. S.
Publikováno v:
Journal of Geophysical Research. Space Physics; 1999, Vol. 104 Issue A2, p2559-2561, 3p
Autor:
R. C. Ygbuhay, H. S. Ahluwalia
Publikováno v:
Solar Physics. 290:635-643
Galactic cosmic-ray (GCR) modulation at 1 AU for sunspot (SSN) Cycle 24 is studied using data from a global network of detectors and balloon measurements of low-energy ions at high latitudes in Russia. The observed modulation is modest compared with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5369599aaf43429413011c19969f17ee
https://doi.org/10.1007/s11207-014-0624-5
https://doi.org/10.1007/s11207-014-0624-5
Publikováno v:
Solar Physics. 289:1763-1782
The pressure corrected hourly data from the global network of cosmic ray detectors, measurements of the interplanetary magnetic field (IMF) intensity (B) at Earth’s orbit and its components B x , B y , B z (in the geocentric solar ecliptic coordina
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::40458e55df59492f82a666367fb1a264
https://doi.org/10.1007/s11207-013-0439-9
https://doi.org/10.1007/s11207-013-0439-9
Autor:
H. S. Ahluwalia
Publikováno v:
Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa5113960848e9494e72b38c6eae29f8
https://doi.org/10.22323/1.236.0102
https://doi.org/10.22323/1.236.0102