M. H. Acuña
About
In The Last Decade
M. H. Acuña
245 papers receiving 16.0k citations
Hit Papers
Peers
Comparison fields: 5 of 96
- Astronomy and Astrophysics 17.0k
- Molecular Biology 6.9k
- Geophysics 1.4k
- Atmospheric Science 1.2k
- Nuclear and High Energy Physics 484
Countries citing papers authored by M. H. Acuña
This map shows the geographic impact of M. H. Acuña'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 M. H. Acuña with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. H. Acuña more than expected).
Fields of papers citing papers by M. H. Acuña
This network shows the impact of papers produced by M. H. Acuña. 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 M. H. Acuña. The network helps show where M. H. Acuña may publish in the future.
Co-authorship network of co-authors of M. H. Acuña
This figure shows the co-authorship network connecting the top 25 collaborators of M. H. Acuña. A scholar is included among the top collaborators of M. H. Acuña 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 M. H. Acuña. M. H. Acuña is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Evidence for Collisionless Magnetic Reconnection at Mars | 2 |
| 2 | Downward Continuation of the Martian Magnetic Field | 1 |
| 3 | Evidence for a Second Martian Dynamo from Electron Reflection Magnetometry | 5 |
| 4 | The effect of crustal magnetic fields and the pressure balance in the high latitude ionosphere/atmosphere at Mars | 1 |
| 5 | Characteristics of Mini-Magnetospheres Formed by Paleo-Magnetic Fields of Mars | 1 |
| 6 | Evidence for Demagnetization of the Utopia Impact Basin on Mars | 1 |
| 7 | Measuring Mars' Atmospheric Neutral Density from 160 to 320km altitude with the MGS Electron Reflectometer | 2 |
| 8 | Shock demagnetization of Martian crust | 2 |
| 9 | Magnetic Field Draping Enhancement at Weakly Magnetized Bodies | 2 |
| 10 | Martian Magnetic Topology: Evaluation of Crustal Magnetization and Solar Wind Interaction Models Using MGS MAG Data | 1 |
| 11 | Regional Mapping of the Lunar Crustal Magnetic Field: Correlation of Strong Anomalies with Curvilinear Albedo Markings | 2 |
| 12 | Strong Magnetic Anomalies on the Lunar Near Side | 1 |
| 13 | Mars' Ionosphere: Influence of Crustal Magnetic Fields and Solar Ionizing Radiation | 1 |
| 14 | The VEVA Mission; exploration of Venus volcanoes and atmosphere | 3 |
| 15 | THE NEAR MAGNETIC FIELD INSTRUMENT | 5 |
| 16 | The Viking satellite program: preliminary results from the APL magnetic field experiment. | 1 |
| 17 | Voyager's Measurements of Saturn's Main Magnetic Field. | 1 |
| 18 | THE MAGSAT PRECISION VECTOR MAGNETOMETER | 13 |
| 19 | Jupiter's magnetic tail: Voyager 1 | 1 |
| 20 | The Main Magnetic Field of Jupiter: Pioneer 11 | 1 |
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.