I. MacLaren

525 total citations
12 papers, 324 citations indexed

About

I. MacLaren is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Instrumentation. According to data from OpenAlex, I. MacLaren has authored 12 papers receiving a total of 324 indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Astronomy and Astrophysics, 3 papers in Atomic and Molecular Physics, and Optics and 3 papers in Instrumentation. Recurrent topics in I. MacLaren's work include Astrophysics and Star Formation Studies (4 papers), Stellar, planetary, and galactic studies (4 papers) and Spectroscopy and Laser Applications (3 papers). I. MacLaren is often cited by papers focused on Astrophysics and Star Formation Studies (4 papers), Stellar, planetary, and galactic studies (4 papers) and Spectroscopy and Laser Applications (3 papers). I. MacLaren collaborates with scholars based in United Kingdom, Australia and United States. I. MacLaren's co-authors include A.W. Wolfendale, K. M. Richardson, D. F. Malin, R. S. Ellis, A. W. Wolfendale, W. J. Couch, R. S. Ellis, Richard S. Ellis and David C. Koo and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and International Journal of Remote Sensing.

In The Last Decade

I. MacLaren

12 papers receiving 318 citations

Peers

I. MacLaren
Viktor Zubko United States
G. Wolf-Chase United States
M. Etxaluze United Kingdom
P. M. Sutter United States
G. Magris Venezuela
R. Behrend Switzerland
T. Lunttila Finland
S. Newman United States
Viktor Zubko United States
I. MacLaren
Citations per year, relative to I. MacLaren I. MacLaren (= 1×) peers Viktor Zubko

Countries citing papers authored by I. MacLaren

Since Specialization
Citations

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

Fields of papers citing papers by I. MacLaren

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of I. MacLaren

This figure shows the co-authorship network connecting the top 25 collaborators of I. MacLaren. A scholar is included among the top collaborators of I. MacLaren 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 I. MacLaren. I. MacLaren is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

12 of 12 papers shown
1.
MacLaren, I., et al.. (2000). Neural network based methods for cloud classification on AVHRR images. International Journal of Remote Sensing. 21(8). 1693–1708. 20 indexed citations
2.
MacLaren, I., et al.. (1994). <title>Neural networks and cloud classification</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 2315. 2–11. 3 indexed citations
3.
Ellis, R. S., et al.. (1991). A uniformly selected catalogue of distant galaxy clusters. Monthly Notices of the Royal Astronomical Society. 249(4). 606–628. 38 indexed citations
4.
MacLaren, I., et al.. (1990). Dust-to-gas ratio and metallicity variations in nearby galaxies. 236(1). 237–241. 5 indexed citations
5.
MacLaren, I. & A. W. Wolfendale. (1990). The 'cosmic ray gradient' and far infrared observations as a tracer of molecular material in the Galaxy. Journal of Physics G Nuclear and Particle Physics. 16(7). 1109–1113. 2 indexed citations
6.
MacLaren, I., et al.. (1990). The size-line width relation and the mass of molecular hydrogen. The Astrophysical Journal. 352. 132–132. 14 indexed citations
7.
MacLaren, I., K. M. Richardson, & A. W. Wolfendale. (1989). Cosmic rays and the masses of giant molecular clouds. Journal of Physics G Nuclear and Particle Physics. 15(8). 1305–1321. 2 indexed citations
8.
MacLaren, I., et al.. (1989). Far-infrared estimates of the mass of gas in the Galaxy. Monthly Notices of the Royal Astronomical Society. 237(4). 1075–1084. 2 indexed citations
9.
MacLaren, I., R. S. Ellis, & W. J. Couch. (1988). Spectral energy distributions of galaxies in high-redshift clusters - III. Abell 370 at z = 0.37. Monthly Notices of the Royal Astronomical Society. 230(2). 249–272. 21 indexed citations
10.
MacLaren, I., et al.. (1988). Dust and the mass of gas in the Galaxy.. 435–439. 1 indexed citations
11.
MacLaren, I., K. M. Richardson, & A.W. Wolfendale. (1988). Corrections to virial estimates of molecular cloud masses. The Astrophysical Journal. 333. 821–821. 212 indexed citations
12.
Ellis, Richard S., W. J. Couch, I. MacLaren, & David C. Koo. (1985). Spectral energy distributions for galaxies in high-redshift clusters – II. 0016 + 16 at z = 0.54. Monthly Notices of the Royal Astronomical Society. 217(2). 239–264. 4 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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