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At the cloud top level of Venus (65-70 km altitude) the atmosphere rotates 60 times faster than the underlying surface, a phenomenon known as superrotation. Whereas on Venus's dayside the cloud top motions are well determined and Venus…

UV-SCOPE is a mission concept to determine the causes of atmospheric mass loss in exoplanets, investigate the mechanisms driving aerosol formation in hot Jupiters, and study the influence of the stellar environment on atmospheric evolution…

Thermal radiation becomes a prominent feature in the continuum spectrum of Venus longwards of $\sim$3 $\mu$m. The emission is traceable to the upper cloud and haze layers in the planet's mesosphere. Venus' thermal radiation spectrum is…

地球与行星天体物理 · 物理学 2024-02-07 A. García Muñoz , P. Wolkenberg , A. Sánchez-Lavega , R. Hueso , I. Garate-Lopez

A moon or natural satellite is a celestial body that orbits a planetary body such as a planet, dwarf planet, or an asteroid. Scientists seek understanding the origin and evolution of our solar system by studying moons of these bodies.…

This PhD thesis consists on a study of the atmospheric dynamics of the planet Venus with data from two space missions separated in time: the Galileo mission and Venus Express. Concretely, images obtained with different wavelengths have been…

地球与行星天体物理 · 物理学 2018-10-15 Javier Peralta

EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^{th}$ of August 2014 from Timmins, Canada. The flight ended…

天体物理仪器与方法 · 物理学 2018-08-09 G. Abdellaoui , S. Abe , J. H. Adams , A. Ahriche , D. Allard , L. Allen , G. Alonso , L. Anchordoqui , A. Anzalone , Y. Arai , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , S. Bacholle , M. Bakiri , P. Baragatti , P. Barrillon , S. Bartocci , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. Belov , K. Belov , K. Benmessai , M. Bertaina , P. L. Biermann , S. Biktemerova , F. Bisconti , N. Blanc , J. Błȩcki , S. Blin-Bondil , P. Bobik , M. Bogomilov , E. Bozzo , A. Bruno , K. S. Caballero , F. Cafagna , D. Campana , J-N. Capdevielle , F. Capel , A. Caramete , L. Caramete , P. Carlson , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , C. Catalano O. Catalano , A. Cellino , M. Chikawa , G. Chiritoi , M. J. Christl , V. Connaughton , L. Conti , G. Cordero , G. Cotto , H. J. Crawford , R. Cremonini , S. Csorna , A. Cummings , S. Dagoret-Campagne , C. De Donato , C. de la Taille , C. De Santis , L. del Peral , M. Di Martino , A. Diaz Damian , T. Djemil , I. Dutan , A. Ebersoldt , T. Ebisuzaki , R. Engel , J. Eser , F. Fenu , S. Fernández-González , J. Fernández-Soriano , S. Ferrarese , M. Flamini , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , J. Fujimoto , M. Fukushima , P. Galeotti , E. García-Ortega , G. Garipov , E. Gascón , J. Genci , G. Giraudo , C. González Alvarado , P. Gorodetzky , R. Greg , F. Guarino , A. Guzmán , Y. Hachisu , M. Haiduc , B. Harlov , A. Haungs , J. Hernández Carretero , W. Hidber Cruz , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , E. Joven , E. G. Judd , A. Jung , J. Jochum , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , Y. Karadzhov , J. Karczmarczyk , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , D. Kolev , H. Krantz , I. Kreykenbohm , K. Kudela , Y. Kurihara , A. Kusenko , E. Kuznetsov , A. La Barbera , C. Lachaud , H. Lahmar , F. Lakhdari , R. Larson , O. Larsson , J. Lee , J. Licandro , L. López Campano , M. C. Maccarone , S. Mackovjak , M. Mahdi , D. Maravilla , L. Marcelli , J. L. Marcos , A. Marini , W. Marszał , K. Martens , Y. Martín , O. Martinez , M. Martucci , G. Masciantonio , K. Mase , M. Mastafa , R. Matev , J. N. Matthews , N. Mebarki , G. Medina-Tanco , M. A. Mendoza , A. Menshikov , A. Merino , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , C. Moretto S. Nagataki , S. Naitamor , T. Napolitano , W. Naslund , R. Nava , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , P. Orleański , G. Osteria , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , G. Pasqualino , E. Parizot , I. H. Park , B. Pastircak , T. Patzak , T. Paul , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , L. Placidi , Z. Plebaniak , S. Pliego , A. Pollini , Z. Polonski , E. M. Popescu , P. Prat , G. Prévôt , H. Prieto , G. Puehlhofer , M. Putis , J. Rabanal , A. A. Radu , M. Reyes , M. Rezazadeh , M. Ricci , M. D. Rodríguez Frías , M. Rodencal , F. Ronga , G. Roudil , I. Rusinov , M. Rybczyński , M. D. Sabau , G. Sáez Cano , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. C. Sanchez Balanzar , J. L. Sánchez , A. Santangelo , A. Sanz-Andrés , M. Sanz Palomino , O. Saprykin , F. Sarazin , M. Sato , T. Schanz , H. Schieler , V. Scotti , S. Selmane , D. Semikoz , M. Serra , S. Sharakin , H. M. Shimizu , K. Shinozaki , T. Shirahama , B. Spataro , I. Stan , T. Sugiyama , D. Supanitsky , M. Suzuki , B. Szabelska , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , H. Takami , M. Takeda , Y. Takizawa , M. C. Talai , C. Tenzer , S. B. Thomas , O. Tibolla , L. Tkachev , H. Tokuno , T. Tomida , N. Tone , S. Toscano , M. Traïche , R. Tsenov , Y. Tsunesada , K. Tsuno , J. Tubbs , S. Turriziani , Y. Uchihori , O. Vaduvescu , J. F. Valdés-Galicia , P. Vallania , G. Vankova , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts , M. Weber , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , Z. Włodarczyk , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S Zgura , M. Yu. Zotov , A. Zuccaro Marchi

The CYGNO project has the goal to use a gaseous TPC with optical readout to detect dark matter and solar neutrinos with low energy threshold and directionality. The CYGNO demonstrator will consist of 1 m 3 volume filled with He:CF 4 gas…

The Near Ultraviolet Transient Explorer (NUTEx) is a CubeSat-based near-ultraviolet (NUV) imaging payload designed for transient sky surveys and is currently under development. CubeSats are compact and cost-effective satellite platforms…

Mini-EUSO will observe the Earth in the UV range (300 - 400 nm) offering the opportunity to study a variety of atmospheric events such as Transient Luminous Events (TLEs), meteors and marine bioluminescence. Furthermore it aims to search…

Though the ultraviolet (UV) domain plays a vital role in the studies of astronomical transient events, the UV time-domain sky remains largely unexplored. We have designed a wide-field UV imager that can be flown on a range of available…

天体物理仪器与方法 · 物理学 2018-03-21 Joice Mathew , S. Ambily , Ajin Prakash , Mayuresh Sarpotdar , K. Nirmal , A. G. Sreejith , Margarita Safonova , Jayant Murthy , Noah Brosch

Selected by NASA for an Astrophysics Science SmallSat study, The Virtual Telescope for X-Ray Observations (VTXO) is a small satellite mission being developed by NASAs Goddard Space Flight Center (GSFC) and New Mexico State University…

天体物理仪器与方法 · 物理学 2020-07-21 Kyle Rankin , John Krizmanic , Neerav Shah , Steven Stochaj , Asal Naseri

SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky area in the Southern Hemisphere using more than 2000…

The DragonCam Microscopic Camera is an instrument being developed for NASA's Dragonfly mission [1] to Saturn's moon Titan. The Microscopic Camera will be body-fixed to the Dragonfly vehicle and will image the surface at a distance of about…

天体物理仪器与方法 · 物理学 2026-01-21 M. J. Clark , M. A. Ravine , M. A. Caplinger , B. A. Lindenfeld , J. D. Laramee , R. S. Bronson , A. D. Giglio , B. G. Crowther

DIOS (Diffuse Intergalactic Oxygen Surveyor) is a small satellite aiming for a launch around 2020 with JAXA's Epsilon rocket. Its main aim is a search for warm-hot intergalactic medium with high-resolution X-ray spectroscopy of redshifted…

Balloon-borne telescopes present unique thermal design challenges which are a combination of those present for both space and ground telescopes. At altitudes of 35-40 km, convection effects are minimal and difficult to characterize.…

In this work we consider the task of detecting sheep onboard an unmanned aerial vehicle (UAV) flying at an altitude of 80 m. At this height, the sheep are relatively small, only about 15 pixels across. Although deep learning strategies have…

计算机视觉与模式识别 · 计算机科学 2020-04-07 Farah Sarwar , Anthony Griffin , Saeed Ur Rehman , Timotius Pasang

The aim of the Degenerate Objects around Degenerate Objects (DODO) survey is to search for very low mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs via direct imaging. The direct detection of such companions…

地球与行星天体物理 · 物理学 2011-03-17 E. Hogan , M. R. Burleigh , F. J. Clarke