Search Results - "Häusler, Bernd"

Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation by Ando, Hiroki, Imamura, Takeshi, Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Sugimoto, Norihiko, Takagi, Masahiro, Sagawa, Hideo, Limaye, Sanjay, Matsuda, Yoshihisa, Choudhary, Raj Kumar, Antonita, Maria

“…We present distributions of the zonal-mean temperature and static stability in the Venusian atmosphere obtained from Venus Express and Akatsuki radio…”
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Structure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express by Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Bird, Michael K., Tyler, G. Leonard

“…The European Space Agency Venus Express Radio Science experiment (VeRa) obtained 118 radio occultation measurements of the Venusian atmosphere between July…”
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The Nucleus of comet 67P/Churyumov–Gerasimenko – Part I: The global view – nucleus mass, mass-loss, porosity, and implications by Pätzold, Martin, Andert, Thomas P, Hahn, Matthias, Barriot, Jean-Pierre, Asmar, Sami W, Häusler, Bernd, Bird, Michael K, Tellmann, Silvia, Oschlisniok, Janusz, Peter, Kerstin

“…The radio science experiment RSI on-board Rosetta determined the mass of the nucleus of comet 67P/Churyumov–Gerasimenko at the start of the prime mission from…”
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Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind by Chiba, Shota, Imamura, Takeshi, Tokumaru, Munetoshi, Shiota, Daikou, Matsumoto, Takuma, Ando, Hiroki, Takeuchi, Hiroshi, Murata, Yasuhiro, Yamazaki, Atsushi, Häusler, Bernd, Pätzold, Martin

“…The properties of the coronal plasma at heliocentric distances of 1.5 – 8.9  R ⊙ (solar radii) were studied with radio-occultation observations using JAXA’s…”
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The lower dayside ionosphere of Mars from 14 years of MaRS radio science observations by Peter, Kerstin, Pätzold, Martin, Molina-Cuberos, Gregorio J., González-Galindo, Francisco, Witasse, Olivier, Tellmann, Silvia, Häusler, Bernd, Bird, Michael K.

“…This work uses a subset of “quiet” MaRS ionospheric dayside observations (MaRSquiet, 2004–2017) and a 1-D photochemical model (IonA-2) to investigate the…”
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The structure of Mars lower atmosphere from Mars Express Radio Science (MaRS) occultation measurements by Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Hinson, D. P., Tyler, G. Leonard

“…The Mars Express Radio Science Experiment (MaRS) investigates the lower and middle atmosphere of Mars between the surface and about 40 km with a very high…”
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RADIAL DISTRIBUTION OF COMPRESSIVE WAVES IN THE SOLAR CORONA REVEALED BY AKATSUKI RADIO OCCULTATION OBSERVATIONS by Miyamoto, Mayu, Imamura, Takeshi, Tokumaru, Munetoshi, Ando, Hiroki, Isobe, Hiroaki, Asai, Ayumi, Shiota, Daikou, Toda, Tomoaki, Hausler, Bernd, Patzold, Martin, NABATOV, ALEXANDER, Nakamura, Masato

“…Radial variations of the amplitude and the energy flux of compressive waves in the solar corona were explored for the first time using a spacecraft radio…”
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A clear view of the multifaceted dayside ionosphere of Mars by Withers, Paul, Fallows, Kathryn, Girazian, Zachary, Matta, Majd, Häusler, Bernd, Hinson, David, Tyler, Len, Morgan, David, Pätzold, Martin, Peter, Kerstin, Tellmann, Silvia, Peralta, Javier, Witasse, Oliver

“…By examining electron density profiles from the Mars Express Radio Science Experiment MaRS, we show that the vertical structure of the dayside ionosphere of…”
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OUTFLOW STRUCTURE OF THE QUIET SUN CORONA PROBED BY SPACECRAFT RADIO SCINTILLATIONS IN STRONG SCATTERING by Imamura, Takeshi, Tokumaru, Munetoshi, Isobe, Hiroaki, Shiota, Daikou, Ando, Hiroki, Miyamoto, Mayu, Toda, Tomoaki, Hausler, Bernd, Patzold, Martin, NABATOV, ALEXANDER, Asai, Ayumi, Yaji, Kentaro, Yamada, Manabu, Nakamura, Masato

“…Radio scintillation observations have been unable to probe flow speeds in the low corona where the scattering of radio waves is exceedingly strong. Here we…”
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Vertical structure of the axi‐asymmetric temperature disturbance in the Venusian polar atmosphere: Comparison between radio occultation measurements and GCM results by Ando, Hiroki, Imamura, Takeshi, Sugimoto, Norihiko, Takagi, Masahiro, Kashimura, Hiroki, Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Matsuda, Yoshihisa

“…Vertical temperature profiles at 40–75 km around 80°N in the Venus polar vortex are retrieved over 13 Earth days almost continuously from radio occultation…”
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Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results by Ando, Hiroki, Takagi, Masahiro, Fukuhara, Tetsuya, Imamura, Takeshi, Sugimoto, Norihiko, Sagawa, Hideo, Noguchi, Katsuyuki, Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Murata, Yasuhiro, Takeuchi, Hiroshi, Yamazaki, Atsushi, Toda, Tomoaki, Tomiki, Atsushi, Choudhary, Rajkumar, Kumar, Kishore, Ramkumar, Geetha, Antonita, Maria

“…Temperature profiles of the Venus atmosphere obtained by the Akatsuki radio occultation measurements showed a prominent local time dependence above 65‐km…”
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Venus Express bistatic radar: High-elevation anomalous reflectivity by Simpson, Richard A., Tyler, G. Leonard, Häusler, Bernd, Mattei, Riccardo, Pätzold, Martin

“…Magellan (MGN) bistatic radar observations in 1994 confirmed earlier Pioneer Venus reports of unusual Venus surface reflectivity and emissivity at elevations…”
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Fine Vertical Structures at the Cloud Heights of Venus Revealed by Radio Holographic Analysis of Venus Express and Akatsuki Radio Occultation Data by Imamura, Takeshi, Miyamoto, Mayu, Ando, Hiroki, Häusler, Bernd, Pätzold, Martin, Tellmann, Silvia, Tsuda, Toshitaka, Aoyama, Yuichi, Murata, Yasuhiro, Takeuchi, Hiroshi, Yamazaki, Atsushi, Toda, Tomoaki, Tomiki, Atsushi

“…Radio occultation (RO) is one of the most efficient techniques for studying fine vertical structures in planetary atmospheres. However, the geometrical optics…”
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Radio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter Akatsuki by Imamura, Takeshi, Toda, Tomoaki, Tomiki, Atsushi, Hirahara, Daichi, Hayashiyama, Tomoko, Mochizuki, Nanako, Yamamoto, Zen-ichi, Abe, Takumi, Iwata, Takahiro, Noda, Hirotomo, Futaana, Yoshifumi, Ando, Hiroki, Häusler, Bernd, Pätzold, Martin, Nabatov, Alexander

“…The Radio Science experiment (RS) in the Akatsuki mission of JAXA aims to determine the vertical structure of the Venus atmosphere, thereby complementing the…”
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Rosetta Radio Science Investigations (RSI) by Paetzold, Martin, Haeusler, Bernd, Aksnes, Kaare, Anderson, John D, Asmar, Sami W, Barriot, Jean-Pierre, Bird, Michael K, Boehnhardt, Hermann, Eidel, Werner, Gruen, Eberhardt, Ip, Wing H, Marouf, Essam, Morley, Trevor, Neubauer, Fritz M, Rickman, Hans, Thomas, Nicolas, Tsurutani, Bruce T, Wallis, Max K, Wickramasinghe, N C, Mysen, Eirik, Olson, Oystein, Remus, Stefan, Tellmann, Silvia, Andert, Thomas, Carone, Ludmila, Fels, Markus, Stanzel, Christina, Audenrieth-Kersten, Iris, Gahr, Alexander, Mueller, Anna-Liane, Stupar, Dusan, Walter, Christina

“…The Rosetta spacecraft has been successfully launched on 2nd March 2004 to its new target comet 67 P/Churyumov-Gerasimenko. The science objectives of the…”
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Coronal Density Structures and CMEs: Superior Solar Conjunctions of Mars Express, Venus Express, and Rosetta: 2004, 2006, and 2008 by Pätzold, Martin, Hahn, Matthias, Tellmann, Silvia, Häusler, Bernd, Bird, Michael K., Tyler, G. Leonard, Asmar, Sami W., Tsurutani, Bruce T.

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OUTFLOW STRUCTURE OF THE QUIET SUN CORONA PROBED BY SPACECRAFT RADIO SCINTILLATIONS IN STRONG SCATTERING by Imamura, Takeshi, Tokumaru, Munetoshi, Isobe, Hiroaki, Shiota, Daikou, Ando, Hiroki, Miyamoto, Mayu, Toda, Tomoaki, Häusler, Bernd, Pätzold, Martin, Nabatov, Alexander, Asai, Ayumi, Yaji, Kentaro, Yamada, Manabu, Nakamura, Masato

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Determination of local surface properties using Mars Express bistatic radar by Simpson, Richard A., Tyler, G. Leonard, Pätzold, Martin, Häusler, Bernd

“…Dual‐frequency bistatic radar experiments were conducted with Mars Express at a rate of one to two per month during 2005. Each observation provided power…”
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Correction to: Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind by Chiba, Shota, Imamura, Takeshi, Tokumaru, Munetoshi, Shiota, Daikou, Matsumoto, Takuma, Ando, Hiroki, Takeuchi, Hiroshi, Murata, Yasuhiro, Yamazaki, Atsushi, Häusler, Bernd, Pätzold, Martin

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Gravity Wave Packets in the Venusian Atmosphere Observed by Radio Occultation Experiments: Comparison With Saturation Theory by Mori, Ryota, Imamura, Takeshi, Ando, Hiroki, Häusler, Bernd, Pätzold, Martin, Tellmann, Silvia

“…The characteristics of gravity wave packets in the Venusian atmosphere were studied using high‐vertical‐resolution temperature profiles obtained by ESA's Venus…”
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