G. Pizzella

2.9k total citations
114 papers, 1.2k citations indexed

About

G. Pizzella is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, G. Pizzella has authored 114 papers receiving a total of 1.2k indexed citations (citations by other indexed papers that have themselves been cited), including 89 papers in Astronomy and Astrophysics, 30 papers in Nuclear and High Energy Physics and 21 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in G. Pizzella's work include Pulsars and Gravitational Waves Research (65 papers), Astrophysics and Cosmic Phenomena (22 papers) and Radio Astronomy Observations and Technology (19 papers). G. Pizzella is often cited by papers focused on Pulsars and Gravitational Waves Research (65 papers), Astrophysics and Cosmic Phenomena (22 papers) and Radio Astronomy Observations and Technology (19 papers). G. Pizzella collaborates with scholars based in Italy, United States and Switzerland. G. Pizzella's co-authors include A. Egidi, U. Amaldi, G. V. Pallottino, G. V. Pallottino, P. Bonifazi, E. Coccia, I. Modena, C. E. McIlwain, E. Amaldi and C. Cosmelli and has published in prestigious journals such as Nature, Journal of Geophysical Research Atmospheres and Annals of the New York Academy of Sciences.

In The Last Decade

G. Pizzella

101 papers receiving 1.0k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
G. Pizzella Italy 18 827 366 253 139 109 114 1.2k
S. Bell United Kingdom 11 856 1.0× 121 0.3× 337 1.3× 142 1.0× 136 1.2× 26 1.2k
M. A. Walker Australia 24 1.2k 1.4× 637 1.7× 651 2.6× 69 0.5× 117 1.1× 83 1.8k
S. Ichimaru Japan 18 1.0k 1.2× 361 1.0× 434 1.7× 78 0.6× 295 2.7× 59 1.6k
Paul Murdin United Kingdom 19 1.3k 1.5× 132 0.4× 422 1.7× 78 0.6× 149 1.4× 110 1.5k
R. Krotkov United States 16 441 0.5× 594 1.6× 169 0.7× 111 0.8× 33 0.3× 30 1.1k
M. C. Weisskopf United States 16 1.1k 1.3× 188 0.5× 589 2.3× 105 0.8× 246 2.3× 63 1.5k
S. Cuperman Israel 18 902 1.1× 200 0.5× 273 1.1× 24 0.2× 144 1.3× 145 1.2k
K. L. Jones Australia 17 462 0.6× 375 1.0× 80 0.3× 34 0.2× 383 3.5× 70 1.3k
A. A. Vasiliev Russia 20 578 0.7× 214 0.6× 115 0.5× 72 0.5× 244 2.2× 59 1.1k
J. A. Lipa United States 19 231 0.3× 560 1.5× 146 0.6× 242 1.7× 83 0.8× 70 1.1k

Countries citing papers authored by G. Pizzella

Since Specialization
Citations

This map shows the geographic impact of G. Pizzella's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by G. Pizzella with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Pizzella more than expected).

Fields of papers citing papers by G. Pizzella

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Pizzella. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by G. Pizzella. The network helps show where G. Pizzella may publish in the future.

Co-authorship network of co-authors of G. Pizzella

This figure shows the co-authorship network connecting the top 25 collaborators of G. Pizzella. A scholar is included among the top collaborators of G. Pizzella based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with G. Pizzella. G. Pizzella is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Astone, P., M. Bassan, E. Coccia, et al.. (2013). Analysis of 3 years of data from the gravitational wave detectors EXPLORER and NAUTILUS. Physical review. D. Particles, fields, gravitation, and cosmology. 87(8). 3 indexed citations
2.
3.
Babusci, D., G. Giordano, G.P. Murtas, & G. Pizzella. (2004). Considerations on coincidence experiments between two gravitational wave detectors for sources in the Galactic Centre. Astronomy and Astrophysics. 421(3). 811–813.
4.
Casale, Monica, et al.. (2002). Performances of Insulation Systems for Inverter-Fed Traction Motors. 148–151. 3 indexed citations
5.
Astone, P., M. Bassan, P. Bonifazi, et al.. (2001). Search for periodic gravitational wave sources with the Explorer detector. Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields. 65(2). 16 indexed citations
6.
Pizzella, G., et al.. (1999). Insulation Systems for Inverter-Fed Traction Motors: A Comparison of the Behaviour of Different Polyimide-Based Composites. European Conference on Power Electronics and Applications. 1–7. 1 indexed citations
7.
Coccia, E., G. Pizzella, & G. Veneziano. (1998). Second Edoardo Amaldi Conference on Gravitational Waves, CERN, Switzerland, 1-4 July 1997. WORLD SCIENTIFIC eBooks. 1 indexed citations
8.
Modestino, G. & G. Pizzella. (1997). Algorithms for correlation analysis between gamma-bursts and gravitational wave data. NASA STI/Recon Technical Report N. 98. 11511. 1 indexed citations
9.
Astone, P., et al.. (1997). The fast matched filter for gravitational-wave data analysis: Characteristics and applications. CNR Solar (Scientific Open-access Literature Archive and Repository) (Consiglio Nazionale delle Ricerche). 20(1). 9–60. 4 indexed citations
10.
Amaldi, E., P. Bonifazi, M. G. Castellano, et al.. (1987). Data recorded by the Rome room temperature gravitational wave antenna, during the supernova SN 1987 A in the Large Magellanic Cloud. NASA STI/Recon Technical Report N. 88. 14922.
11.
Amaldi, E., P. Bonifazi, P. Carelli, et al.. (1987). Operation of the 2270 kg gravitational wave resonant antenna of the Rome group.. 18.
12.
Pizzella, G.. (1984). The Search for Gravitational Waves. Physics Bulletin. 35(12). 508–510. 3 indexed citations
13.
Amaldi, E., P. Bonifazi, F. Bronzini, et al.. (1983). The gravitational wave experiment of the Rome group.. CERN Bulletin. 499–521. 5 indexed citations
14.
Pizzella, G.. (1977). The cryogenic gravitational wave experiment in Rome: progress report. General Relativity and Gravitation. 49. 2 indexed citations
15.
Pallottino, G. V. & G. Pizzella. (1977). Electrical equivalent circuits of multiple-sensor gravitational-wave antennas. STIN. 78. 14284. 1 indexed citations
16.
D’Anna, E., G. Pizzella, & D. Trèvese. (1974). Cross-sections of a cylindrical antenna for gravitational waves. Lettere al nuovo cimento della societa italiana di fisica/Lettere al nuovo cimento. 9(6). 231–234. 1 indexed citations
17.
Pizzella, G., et al.. (1973). Evidence for emission of cosmic rays by Jupiter. ICRC. 2. 1129–1134. 2 indexed citations
18.
Pizzella, G.. (1970). Emission of Cosmic Rays by a Dipole Magnetosphere. Nature. 226(5244). 434–435.
19.
Forbush, Scott E., G. Pizzella, & D. Venkatesan. (1962). The morphology and temporal variations of the Van Allen radiation belt, October 1959 to December 1960. Journal of Geophysical Research Atmospheres. 67(10). 3651–3668. 52 indexed citations
20.
Pizzella, G., C. E. McIlwain, & J. A. Van Allen. (1962). Reply to the Discussion by W. N. Hess [on ‘Time variations of Intensity in the Earth's Inner Radiation Zone, October 1959 through December 1960’]. Journal of Geophysical Research Atmospheres. 67(12). 4888–4889. 2 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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