Found: 15
Select item for more details and to access through your institution.
Correction to: Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind.
- Published in:
- 2023
- By:
- Publication type:
- Correction Notice
Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements.
- Published in:
- Journal of Geophysical Research. Planets, 2022, v. 127, n. 3, p. 1, doi. 10.1029/2021JE006957
- By:
- Publication type:
- Article
Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind.
- Published in:
- Solar Physics, 2022, v. 297, n. 3, p. 1, doi. 10.1007/s11207-022-01968-9
- By:
- Publication type:
- Article
Gravity Wave Packets in the Venusian Atmosphere Observed by Radio Occultation Experiments: Comparison With Saturation Theory.
- Published in:
- Journal of Geophysical Research. Planets, 2021, v. 126, n. 9, p. 1, doi. 10.1029/2021JE006912
- By:
- Publication type:
- Article
Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results.
- Published in:
- Journal of Geophysical Research. Planets, 2018, v. 123, n. 9, p. 2270, doi. 10.1029/2018JE005640
- By:
- Publication type:
- Article
Fine Vertical Structures at the Cloud Heights of Venus Revealed by Radio Holographic Analysis of Venus Express and Akatsuki Radio Occultation Data.
- Published in:
- Journal of Geophysical Research. Planets, 2018, v. 123, n. 8, p. 2151, doi. 10.1029/2018JE005627
- By:
- Publication type:
- Article
Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki.
- Published in:
- Earth, Planets & Space, 2017, v. 69, n. 1, p. 1, doi. 10.1186/s40623-017-0722-3
- By:
- Publication type:
- Article
Vertical structure of the axi-asymmetric temperature disturbance in the Venusian polar atmosphere: Comparison between radio occultation measurements and GCM results.
- Published in:
- Journal of Geophysical Research. Planets, 2017, v. 122, n. 8, p. 1687, doi. 10.1002/2016JE005213
- By:
- Publication type:
- Article
Vertical Wavenumber Spectra of Gravity Waves in the Venus Atmosphere Obtained from Venus Express Radio Occultation Data: Evidence for Saturation.
- Published in:
- Journal of the Atmospheric Sciences, 2015, v. 72, n. 6, p. 2318, doi. 10.1175/JAS-D-14-0315.1
- By:
- Publication type:
- Article
A clear view of the multifaceted dayside ionosphere of Mars.
- Published in:
- Geophysical Research Letters, 2012, v. 39, n. 18, p. n/a, doi. 10.1029/2012GL053193
- By:
- Publication type:
- Article
Coronal Density Structures and CMEs: Superior Solar Conjunctions of Mars Express, Venus Express, and Rosetta: 2004, 2006, and 2008.
- Published in:
- Solar Physics, 2012, v. 279, n. 1, p. 127, doi. 10.1007/s11207-012-9991-y
- By:
- Publication type:
- Article
Venus Express bistatic radar: High-elevation anomalous reflectivity.
- Published in:
- Journal of Geophysical Research. Planets, 2009, v. 114, n. E9, p. n/a, doi. 10.1029/2008JE003156
- By:
- Publication type:
- Article
Structure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express.
- Published in:
- Journal of Geophysical Research. Planets, 2009, v. 114, n. E9, p. n/a, doi. 10.1029/2008JE003204
- By:
- Publication type:
- Article
Rosetta Radio Science Investigations (RSI).
- Published in:
- Space Science Reviews, 2006, v. 128, n. 1-4, p. 599, doi. 10.1007/s11214-006-9117-7
- By:
- Publication type:
- Article
Determination of local surface properties using Mars Express bistatic radar.
- Published in:
- Journal of Geophysical Research. Planets, 2006, v. 111, n. E6, p. n/a, doi. 10.1029/2005JE002580
- By:
- Publication type:
- Article