Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
The Large Angle Spectroscopic Coronagraph (LASCO)
19951.9k citationsR. A. Howard, M. J. Koomen et al.profile →
Measurements of Flow Speeds in the Corona Between 2 and 30R☉
1997410 citationsR. A. Howard, M. J. Koomen et al.profile →
Citations per year, relative to G. M. Simnett G. M. Simnett (= 1×)
peers
L. A. Fisk
Countries citing papers authored by G. M. Simnett
Since
Specialization
Citations
This map shows the geographic impact of G. M. Simnett'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. M. Simnett with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. M. Simnett more than expected).
This network shows the impact of papers produced by G. M. Simnett. 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. M. Simnett. The network helps show where G. M. Simnett may publish in the future.
Co-authorship network of co-authors of G. M. Simnett
This figure shows the co-authorship network connecting the top 25 collaborators of G. M. Simnett.
A scholar is included among the top collaborators of G. M. Simnett 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. M. Simnett. G. M. Simnett 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.
Simnett, G. M. & S. W. Kahler. (2005). Interplanetary CMEs Without Observed Coronagraph CMEs. CERN Document Server (European Organization for Nuclear Research). 1. 165.2 indexed citations
2.
Kahler, S. W. & G. M. Simnett. (2005). Imaging Interplanetary Disturbances Causing Forbush Decreases. CERN Document Server (European Organization for Nuclear Research). 2. 267.1 indexed citations
3.
Simnett, G. M. & E. C. Roelof. (2005). Timing of the relativistic proton acceleration responsible for the GLE on 20 January, 2005. CERN Document Server (European Organization for Nuclear Research). 1. 233.3 indexed citations
4.
Simnett, G. M. & S. W. Kahler. (2004). Imaging of Interplanetary Disturbances Causing Forbush Decreases. AGU Fall Meeting Abstracts. 2004.1 indexed citations
5.
Simnett, G. M., E. C. Roelof, & D. K. Haggerty. (2001). What Have Impulsive Near-Relativistic Electron Events to do With CMEs?. AGU Spring Meeting Abstracts. 2001.1 indexed citations
6.
Simnett, G. M., E. C. Roelof, & D. K. Haggerty. (2001). The Acceleration and Release of Near-Relativistic Electrons by CMEs. AGUFM. 2001.4 indexed citations
7.
Fisk, L. A., J. R. Jokipii, G. M. Simnett, R. von Steiger, & K. P. Wenzel. (1998). Cosmic Rays in the Heliosphere. CERN Document Server (European Organization for Nuclear Research).14 indexed citations
8.
Simnett, G. M., C. E. Alissandrakis, & L. Vlahos. (1997). Solar and heliospheric plasma physics : proceedings of the 8th European Meeting on Solar Physics, held at Halkidiki, [near Thessaloniki], Greece, 13-18 May, 1996. Springer eBooks.1 indexed citations
9.
Simnett, G. M., R. B. Decker, & E. C. Roelof. (1997). Confinement of Electrons, Accelerated at Distant High Latitude Corotating Interaction Regions, to the Inner Heliosphere. International Cosmic Ray Conference. 1. 361.1 indexed citations
10.
Tappin, S. J. & G. M. Simnett. (1997). The Acceleration of CMEs in the Outer Corona as Revealed by LASCO. ESASP. 415. 117.2 indexed citations
11.
Roelof, E. C., et al.. (1993). Low Energy Ion and Electron Events at Ulysses Beyond 5 AU and at IMP8 near Earth. 3. 338.1 indexed citations
12.
Brueckner, G. E., R. A. Howard, M. J. Koomen, et al.. (1992). The Large Angle Spectroscopic Coronagraph (LASCO): visible light coronal imaging and spectroscopy.. ESASP. 348. 27–34.1 indexed citations
13.
Lanzerotti, L. J., C. G. Maclennan, P. J. White, et al.. (1991). Low Energy Ion and Electron Measurements of the March-April 1991 Solar Events by Ulysses. International Cosmic Ray Conference. 3. 181.1 indexed citations
14.
Schmieder, B., L. van Driel‐Gesztelyi, J. C. Hénoux, & G. M. Simnett. (1991). Conditions for flare and filament formation in interacting solar active regions. 244(2). 533–543.9 indexed citations
15.
Simnett, G. M., et al.. (1980). A Study of the Impulsive Flares and Homologous Flares From AR2372 From April 6-13, Using Hard X-Ray Images. Bulletin of the American Astronomical Society. 12. 899.1 indexed citations
16.
Wilson, J. W., et al.. (1979). The control of a hard X-ray imaging spectrometer on board the SMM using two mutually redundant microprocessors. Journal of the British Interplanetary Society. 32. 70–76.
17.
Simnett, G. M., et al.. (1973). A search for solar neutrons from 10-100 MeV. International Cosmic Ray Conference. 2. 1583.
18.
White, R. S., et al.. (1972). Earth albedo and solar neutrons.. 2. 683–687.21 indexed citations
19.
Simnett, G. M.. (1972). Relativistic electrons in space.. NASA Technical Reports Server (NASA). 2. 745–762.1 indexed citations
20.
Simnett, G. M., T. L. Cline, S. S. Holt, & F. B. McDonald. (1970). Delayed appearance of relativistic electrons 5 days after a solar flare. Acta physica Hungarica. 2. 649–656.3 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.