The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where H. K. Eriksen sits on this spectrum.
This scientist: 503 publications — 56th percentile
56% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where H. K. Eriksen sits on this spectrum.
This scientist: 165 D-Index — 95th percentile
95% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
H. K. Eriksen is affiliated with the University of Oslo in Norway and has made significant contributions to the field of Physics and Astronomy, particularly within Astronomy and Astrophysics. Their research portfolio encompasses a broad range of topics including Cosmology and Gravitation Theories, Radio Astronomy Observations and Technology, and Galaxies: Formation, Evolution, Phenomena.
Their notable recent papers include:
Their frequent co-authors across multiple publications are:
Eriksen has published mainly in the following venues:
Detailed publication data reveals an active research presence with a total of 41 publications in Astronomy and Astrophysics, the core subfield that aligns with their main scientific focus. Additional subfields of interest include Oceanography, Nuclear and High Energy Physics, Statistical and Nonlinear Physics, and Aerospace Engineering.
The main topics of Eriksen's work range from deep theoretical studies in Cosmology and Gravitation Theories to practical applications and observational techniques in Radio Astronomy. Other research areas comprise Geophysics and Gravity Measurements, Solar and Space Plasma Dynamics, Superconducting and THz Device Technology, and Dark Matter and Cosmic Phenomena.
P. A. R. Ade;N. Aghanim;M. Arnaud
Peter A. R. Ade;N. Aghanim;M. Arnaud;M. Ashdown
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan
P. A. R. Ade;N. Aghanim;M. Arnaud
N. Aghanim;Y. Akrami;Y. Akrami;Y. Akrami;M. Ashdown
N. Aghanim;Y. Akrami;Y. Akrami;Y. Akrami;M. I. R. Alves;M. I. R. Alves;M. I. R. Alves
P.A.R. Ade;N. Aghanim;M. Arnaud;F. Arroja;F. Arroja
P. A. R. Ade;N. Aghanim;M. I. R. Alves
P.A.R. Ade;F.X. Desert;J. Knoche;M. Giard
P. A. R. Ade;N. Aghanim;M. Arnaud;M. Ashdown
Y. Akrami;F. Arroja;M. Ashdown
P. A. R. Ade;N. Aghanim;M. Arnaud
N. Aghanim;M. Arnaud;M. Ashdown
P. A. R. Ade;N. Aghanim;Z. Ahmed;R. W. Aikin
P. A. R. Ade;N. Aghanim;M. Arnaud
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan
R. Adam;P. A. R. Ade;N. Aghanim
N. Aghanim;M. Arnaud;M. Ashdown;J. Aumont
P. A. R. Ade;N. Aghanim;C. Armitage-Caplan
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