G. Moreno

1.8k total citations
68 papers, 1.4k citations indexed

About

G. Moreno is a scholar working on Astronomy and Astrophysics, Molecular Biology and Oceanography. According to data from OpenAlex, G. Moreno has authored 68 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 66 papers in Astronomy and Astrophysics, 22 papers in Molecular Biology and 9 papers in Oceanography. Recurrent topics in G. Moreno's work include Solar and Space Plasma Dynamics (54 papers), Ionosphere and magnetosphere dynamics (37 papers) and Astro and Planetary Science (27 papers). G. Moreno is often cited by papers focused on Solar and Space Plasma Dynamics (54 papers), Ionosphere and magnetosphere dynamics (37 papers) and Astro and Planetary Science (27 papers). G. Moreno collaborates with scholars based in Italy, United States and Cuba. G. Moreno's co-authors include C. Bonifazi, V. Formisano, F. Palmiotto, P. C. Hedgecock, M. B. Bavassano Cattaneo, J. D. Richardson, A. Egidi, M. Dobrowolny, M. Storini and S. Orsini and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Geophysical Research Letters.

In The Last Decade

G. Moreno

67 papers receiving 975 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. Moreno Italy 20 1.4k 368 232 165 146 68 1.4k
J. Fainberg United States 26 2.1k 1.5× 466 1.3× 260 1.1× 198 1.2× 99 0.7× 107 2.2k
P. C. Hedgecock United Kingdom 18 1.8k 1.3× 769 2.1× 359 1.5× 147 0.9× 153 1.0× 35 1.9k
R. J. Fitzenreiter United States 24 1.9k 1.4× 605 1.6× 282 1.2× 174 1.1× 137 0.9× 56 1.9k
Michael D. Montgomery United States 15 1.1k 0.8× 287 0.8× 184 0.8× 145 0.9× 111 0.8× 17 1.2k
M. L. Goldstein United States 13 1.1k 0.8× 371 1.0× 81 0.3× 98 0.6× 97 0.7× 26 1.1k
E. Amata Italy 23 1.4k 1.0× 612 1.7× 315 1.4× 151 0.9× 54 0.4× 77 1.5k
K.‐H. Mühlhäuser Germany 14 2.2k 1.6× 461 1.3× 117 0.5× 126 0.8× 186 1.3× 21 2.2k
M. L. Kaiser United States 21 2.0k 1.5× 426 1.2× 139 0.6× 116 0.7× 48 0.3× 53 2.0k
V. A. Osherovich United States 19 1.3k 0.9× 510 1.4× 154 0.7× 94 0.6× 55 0.4× 89 1.3k
G. Belmont France 26 1.9k 1.4× 830 2.3× 187 0.8× 364 2.2× 102 0.7× 74 2.0k

Countries citing papers authored by G. Moreno

Since Specialization
Citations

This map shows the geographic impact of G. Moreno'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. Moreno with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Moreno more than expected).

Fields of papers citing papers by G. Moreno

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Moreno. 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. Moreno. The network helps show where G. Moreno may publish in the future.

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

This figure shows the co-authorship network connecting the top 25 collaborators of G. Moreno. A scholar is included among the top collaborators of G. Moreno 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. Moreno. G. Moreno 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.
Laurenza, Monica, et al.. (2008). Characteristic Features of the 11-Year Cycle in Cosmic Ray Data. International Cosmic Ray Conference. 1. 513–516. 2 indexed citations
2.
Laurenza, Monica, M. Storini, G. Moreno, & Z. Fujii. (2004). Reliability of the interplanetary magnetic field polarities inferred from north‐south cosmic ray anisotropy and geomagnetic data. Journal of Geophysical Research Atmospheres. 109(A6). 2 indexed citations
3.
Landi, R., et al.. (1998). Coronal mass ejections, flares, and geomagnetic storms. Journal of Geophysical Research Atmospheres. 103(A9). 20553–20559. 13 indexed citations
4.
Orlando, Maria Patrizia, G. Moreno, Miranda Parisi, & M. Storini. (1995). Diurnal modulation of the geomagnetic activity induced by the southward component of the interplanetary magnetic field. Journal of Geophysical Research Atmospheres. 100(A10). 19565–19570. 10 indexed citations
5.
Moreno, G., et al.. (1993). Are there fast-rotating giant active longitudes ?. Solar Physics. 144(2). 399–402. 6 indexed citations
6.
Petris, M. De, M. Gervasi, S. Masi, et al.. (1991). Interplanetary perturbation-induced effects on polar ozone level. Annales Geophysicae. 9(6). 381–386. 4 indexed citations
7.
Cattaneo, M. B. Bavassano, P. W. Cattaneo, G. Moreno, & R. P. Lepping. (1991). Upstream waves in Saturn's foreshock. Geophysical Research Letters. 18(5). 797–800. 7 indexed citations
8.
Petris, M. De, et al.. (1990). On the Antarctic ozone depletion during solar cycle 21. Annales Geophysicae. 8. 541–547. 2 indexed citations
9.
Bernardis, P. de, et al.. (1989). Infrared emission from interplanetary dust. The Astrophysical Journal. 337. 528–528. 3 indexed citations
10.
Salama, A., P. Andreani, G. Dall’Oglio, et al.. (1987). Measurements of near- and far-infrared zodiacal dust emission. The Astronomical Journal. 93. 467–467. 5 indexed citations
11.
Bavassano‐Cattaneo, M. B., et al.. (1987). Observations of large‐amplitude MHD waves in Jupiter's foreshock in connection with a quasi‐perpendicular shock structure. Journal of Geophysical Research Atmospheres. 92(A11). 12413–12418. 7 indexed citations
12.
Bonifazi, C. & G. Moreno. (1981). Reflected and diffuse ions backstreaming from the Earth's bow shock 1. Basic properties. Journal of Geophysical Research Atmospheres. 86(A6). 4397–4404. 99 indexed citations
13.
Bonifazi, C., G. Moreno, A. J. Lazarus, & J. D. Sullivan. (1980). Deceleration of the solar wind in the Earth's foreshock region: Isee 2 and Imp 8 observations. Journal of Geophysical Research Atmospheres. 85(A11). 6031–6038. 53 indexed citations
14.
Formisano, V., S. Orsini, C. Bonifazi, A. Egidi, & G. Moreno. (1980). High time resolution observations of the solar wind and backstreaming ions in the Earth’s foreshock region. Geophysical Research Letters. 7(5). 385–388. 11 indexed citations
15.
Bavassano‐Cattaneo, M. B., C. Bonifazi, P. Cerulli‐Irelli, et al.. (1979). Preliminary results from the solar wind experiment on the ISEE-2 satellite. Space Science Reviews. 23(1). 12 indexed citations
16.
Moreno, G., et al.. (1977). A two-spacecraft study of the preshock perturbations of the solar wind protons. Journal of Geophysical Research Atmospheres. 82(25). 3615–3622. 13 indexed citations
17.
Moreno, G., et al.. (1974). Long-term variations of the solar wind proton parameters. Journal of Geophysical Research Atmospheres. 79(34). 5095–5108. 45 indexed citations
18.
Formisano, V., P. C. Hedgecock, G. Moreno, F. Palmiotto, & J. K. Chao. (1973). Solar wind interaction with the Earth's magnetic field: 2. Magnetohydrodynamic bow shock. Journal of Geophysical Research Atmospheres. 78(19). 3731–3744. 68 indexed citations
19.
Formisano, V., et al.. (1972). HEOS 1 helium observations in the solar wind. NASA Technical Reports Server (NASA). 308. 588. 20 indexed citations
20.
Formisano, V., A. Egidi, & G. Moreno. (1970). Observation of solar-wind α-particles in the magnetosheath. Lettere al nuovo cimento della societa italiana di fisica/Lettere al nuovo cimento. 3(7). 209–212. 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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