The cosmic ray (CR) intensity data recorded with Deep River Neutron Monitoring Station have been investigated on quietest days (QD) for higher harmonics of daily variation during solar cycle 21 and 22. It has been observed that inspite of the abrupt change in the amplitude and phase of tri-diurnal and quart diurnal anisotropy in CR intensity, the amplitude of third harmonic is quite significant throughout the period of investigation with larger amplitude during the year 1980 and 1985. Thus, tri-diurnal anisotropy clearly shows 11 year variation at mid latitude neutron monitoring station.
Published in |
International Journal of Astrophysics and Space Science (Volume 3, Issue 2-1)
This article belongs to the Special Issue Modulation of Cosmic Rays, Inter Planetary Magnetic Field, Magnetic Storm, Large and Small Amplitude Wave Train |
DOI | 10.11648/j.ijass.s.2015030201.12 |
Page(s) | 4-6 |
Creative Commons |
This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited. |
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Copyright © The Author(s), 2015. Published by Science Publishing Group |
Cosmic Rays/ Higher Harmonics/Geo-magnetically Quiet Days
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APA Style
M. K. Richharia. (2015). Study of Higher Harmonics of Cosmic Ray Intensity on Quiet Days at Deep River Neutron Monitoring Station. International Journal of Astrophysics and Space Science, 3(2-1), 4-6. https://doi.org/10.11648/j.ijass.s.2015030201.12
ACS Style
M. K. Richharia. Study of Higher Harmonics of Cosmic Ray Intensity on Quiet Days at Deep River Neutron Monitoring Station. Int. J. Astrophys. Space Sci. 2015, 3(2-1), 4-6. doi: 10.11648/j.ijass.s.2015030201.12
AMA Style
M. K. Richharia. Study of Higher Harmonics of Cosmic Ray Intensity on Quiet Days at Deep River Neutron Monitoring Station. Int J Astrophys Space Sci. 2015;3(2-1):4-6. doi: 10.11648/j.ijass.s.2015030201.12
@article{10.11648/j.ijass.s.2015030201.12, author = {M. K. Richharia}, title = {Study of Higher Harmonics of Cosmic Ray Intensity on Quiet Days at Deep River Neutron Monitoring Station}, journal = {International Journal of Astrophysics and Space Science}, volume = {3}, number = {2-1}, pages = {4-6}, doi = {10.11648/j.ijass.s.2015030201.12}, url = {https://doi.org/10.11648/j.ijass.s.2015030201.12}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.s.2015030201.12}, abstract = {The cosmic ray (CR) intensity data recorded with Deep River Neutron Monitoring Station have been investigated on quietest days (QD) for higher harmonics of daily variation during solar cycle 21 and 22. It has been observed that inspite of the abrupt change in the amplitude and phase of tri-diurnal and quart diurnal anisotropy in CR intensity, the amplitude of third harmonic is quite significant throughout the period of investigation with larger amplitude during the year 1980 and 1985. Thus, tri-diurnal anisotropy clearly shows 11 year variation at mid latitude neutron monitoring station.}, year = {2015} }
TY - JOUR T1 - Study of Higher Harmonics of Cosmic Ray Intensity on Quiet Days at Deep River Neutron Monitoring Station AU - M. K. Richharia Y1 - 2015/03/18 PY - 2015 N1 - https://doi.org/10.11648/j.ijass.s.2015030201.12 DO - 10.11648/j.ijass.s.2015030201.12 T2 - International Journal of Astrophysics and Space Science JF - International Journal of Astrophysics and Space Science JO - International Journal of Astrophysics and Space Science SP - 4 EP - 6 PB - Science Publishing Group SN - 2376-7022 UR - https://doi.org/10.11648/j.ijass.s.2015030201.12 AB - The cosmic ray (CR) intensity data recorded with Deep River Neutron Monitoring Station have been investigated on quietest days (QD) for higher harmonics of daily variation during solar cycle 21 and 22. It has been observed that inspite of the abrupt change in the amplitude and phase of tri-diurnal and quart diurnal anisotropy in CR intensity, the amplitude of third harmonic is quite significant throughout the period of investigation with larger amplitude during the year 1980 and 1985. Thus, tri-diurnal anisotropy clearly shows 11 year variation at mid latitude neutron monitoring station. VL - 3 IS - 2-1 ER -