L. P. Giver
About
In The Last Decade
L. P. Giver
50 papers receiving 614 citations
Peers
Comparison fields: 5 of 39
- Spectroscopy 451
- Atmospheric Science 410
- Global and Planetary Change 219
- Astronomy and Astrophysics 175
- Electrical and Electronic Engineering 124
Countries citing papers authored by L. P. Giver
This map shows the geographic impact of L. P. Giver'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 L. P. Giver with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. P. Giver more than expected).
Fields of papers citing papers by L. P. Giver
This network shows the impact of papers produced by L. P. Giver. 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 L. P. Giver. The network helps show where L. P. Giver may publish in the future.
Co-authorship network of co-authors of L. P. Giver
This figure shows the co-authorship network connecting the top 25 collaborators of L. P. Giver. A scholar is included among the top collaborators of L. P. Giver 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 L. P. Giver. L. P. Giver is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 11 | |
| 3 | 11 | |
| 4 | 10 | |
| 5 | Exponential Sum Fits to Near Infrared Methane Laboratory Spectra at Temperatures of 110 to 295 K | 2 |
| 6 | Constraints on Haze and Cloud Structure from Titan's Albedo Between 1 and 2.5 μm | 2 |
| 7 | First 3-4 Micron Observation of Triton and Pluto | 3 |
| 8 | Band Models of Methane Gas Phase Spectra, 2.1-2.5 μm, Extrapolated to T=55 K for Analysis of Triton's Spectrum | 3 |
| 9 | 36 | |
| 10 | Band Model Coefficients of Methane from 4000 to 9200 cm -1 , Determined at 112, 188, and 294° K | 2 |
| 11 | 14 | |
| 12 | 5 | |
| 13 | Analysis of the CH 4 3ν 3 Bands as Applied to Titan. | 2 |
| 14 | Interpretation of the Red Methane Absorption Bands in the Spectrum of Titan | 1 |
| 15 | Theoretical interpretation of the 0.7820-micron CO2 band and 0.8226-micron H2O line on Venus | 1 |
| 16 | Rotational Temperatures of Venus Derived from Inhomogeneous Scattering Model Atmospheres | 2 |
| 17 | A Comparison of Venus Cloud Models Determined by Spectroscopic Investigations | 2 |
| 18 | 70 | |
| 19 | High-dispersion spectroscopic observations of Mars. II. | 3 |
| 20 | 4 |
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.