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When the Stratospheric Observatory for Infrared Astronomy (SOFIA) was conceived and its first science cases defined, exoplanets had not been detected. Later studies, however, showed that optical and near-infrared photometric and…

Instrumentation and Methods for Astrophysics · Physics 2019-02-06 Daniel Angerhausen

The survey of the nearby space and continuous monitoring of the Near Earth Objects (NEOs) and especially Near Earth Asteroids (NEAs) are essential for the future of our planet and should represent a priority for our solar system research…

The Sun Watcher with Active Pixels and Image Processing (SWAP) is an EUV solar telescope on board ESA's Project for Onboard Autonomy 2 (PROBA2) mission launched on 2 November 2009. SWAP has a spectral bandpass centered on 17.4 nm and…

The calibration of ground-based submillimetre observations has always been a difficult process. We discuss how to overcome the limitations imposed by the submillimetre atmosphere. Novel ways to improve line-of-sight opacity estimates are…

The Solar Orbiter mission, to be launched in July 2017, will carry a suite of remote sensing and in-situ instruments, including the Polarimetric and Helioseismic Imager (PHI). PHI will deliver high-cadence images of the Sun in intensity and…

Technical description of the new project called All Sky Automated Survey and results of the tests of our prototype instrument are presented. The ultimate goal of this project is photometric monitoring of the large area of the sky with fully…

Astrophysics · Physics 2007-05-23 G. Pojmanski

In March 2009, NASA will launch the Kepler satellite -- a mission designed to discover habitable Earth-like planets around distant Sun-like stars. The method that Kepler will use to detect distant worlds will only reveal the size of the…

Astrophysics · Physics 2008-10-14 Travis S. Metcalfe

This study presents a comprehensive system analysis for an instrument onboard the Habitable Worlds Observatory (HWO), designed for high-precision, high-accuracy differential astrometry, with the primary scientific goal to determine the mass…

We present one of the new generations of observatories, the Stratospheric Observatory For Infrared Astronomy (SOFIA). This is an airborne observatory consisting of a 2.7-m telescope mounted on a modified Boeing B747-SP airplane. Flying at…

Instrumentation and Methods for Astrophysics · Physics 2010-10-06 M. Hamidouche , E. Young , P. Marcum , A. Krabbe

Low-frequency radio observations have been expected to serve as a powerful tool for Space Weather (SW) observations for decades. Radio observations are sensitive to a wide range of SW-related observations ranging from emissions from coronal…

Solar and Stellar Astrophysics · Physics 2023-02-01 Devojyoti Kansabanik , Surajit Mondal , Divya Oberoi , Puja Majee

Aerial communication platforms, stratospheric high-altitude platform stations (HAPS), have the potential to provide/catalyze advanced mobile wireless communication services with its ubiquitous connectivity and ultra-wide coverage radius.…

Signal Processing · Electrical Eng. & Systems 2023-03-10 Sidrah Javed , Mohamed-Slim Alouini , Zhiguo Ding

Observations, analysis techniques and photometric properties of a multi-narrowband survey of a 20 square-degree area of sky at +33 degrees declination are described. The survey is conducted with the 3-meter liquid-mirror telescope of the…

Astrophysics · Physics 2007-05-23 Paul Hickson , Mark K. Mulrooney

The possibilities of organizing an observation service for solar activity in order to provide space weather forecasting are considered. The most promising at this stage is the creation of a ground-based observation network. Such a network…

Solar and Stellar Astrophysics · Physics 2023-03-06 A. G. Tlatov , A. A. Pevtsov

An important goal within the quest for detecting an Earth-like extrasolar planet, will be to identify atmospheric gaseous bio-signatures. Observations of the light transmitted through the Earth's atmosphere, as for an extrasolar planet,…

It has been posited that lunar eclipse observations may help predict the in-transit signature of Earth-like extrasolar planets. However, a comparative analysis of the two phenomena addressing in detail the transport of stellar light through…

Solar and Stellar Astrophysics · Physics 2015-06-05 A. García Muñoz , M. R. Zapatero Osorio , R. Barrena , P. Montañés-Rodríguez , E. L. Martín , E. Pallé

Recent advances in miniaturization and commercial availability of critical satellite subsystems and detector technology have made small satellites (SmallSats, including CubeSats) an attractive, low-cost potential solution for space weather…

Instrumentation and Methods for Astrophysics · Physics 2022-02-02 Amir Caspi , M. Barthelemy , C. D. Bussy-Virat , I. J. Cohen , C. E. DeForest , D. R. Jackson , A. Vourlidas , T. Nieves-Chinchilla

A total lunar eclipse is plausible to have an influence on the variation of some environmental physical parameters, specifically on the conditions of the sky brightness, humidity and temperature. During the eclipse on 14$^{th}$-15$^{th}$…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 C. Góez Therán , S. Vargas Domínguez

Beyond the Sun-Earth line, spacecraft equipped with various solar telescopes are intended to be deployed at several different vantage points in the heliosphere to carry out coordinated, multi-view observations of the Sun and its dynamic…

Solar and Stellar Astrophysics · Physics 2024-08-09 Jinsung Lee , Sung-Hong Park , Arik Posner , Kyung-Suk Cho , Jaemyung Ahn

The main goal of this work is the analysis of new approaches to the study of the properties of astronomical sites. In particular, satellite data measuring aerosols have recently been proposed as a useful technique for site characterization…

Astrophysics · Physics 2008-10-07 A. M. Varela , C. Bertolin , C. Muñoz-Tuñón , S. Ortolani , J. J. Fuensalida

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the…

Instrumentation and Methods for Astrophysics · Physics 2024-01-15 EUSO Collaboration , G. Abdellaoui , S. Abe , J. H. Adams. , D. Allard , G. Alonso , L. Anchordoqui , A. Anzalone , E. Arnone , K. Asano , R. Attallah , H. Attoui , M. Ave Pernas , R. Bachmann , S. Bacholle , M. Bagheri , M. Bakiri , J. Baláz , D. Barghini , S. Bartocci , M. Battisti , J. Bayer , B. Beldjilali , T. Belenguer , N. Belkhalfa , R. Bellotti , A. A. Belov , K. Benmessai , M. Bertaina , P. F. Bertone , P. L. Biermann , F. Bisconti , C. Blaksley , N. Blanc , S. Blin-Bondil , P. Bobik , M. Bogomilov , K. Bolmgren , E. Bozzo , S. Briz , A. Bruno , K. S. Caballero , F. Cafagna , G. Cambié , D. Campana , J. N. Capdevielle , F. Capel , A. Caramete , L. Caramete , R. Caruso , M. Casolino , C. Cassardo , A. Castellina , O. Catalano , A. Cellino , K. Černý , M. Chikawa , G. Chiritoi , M. J. Christl , R. Colalillo , L. Conti , G. Cotto , H. J. Crawford , R. Cremonini , A. Creusot , A. Cummings , A. de Castro Gónzalez , C. de la Taille , L. del Peral , J. Desiato , A. Diaz Damian , R. Diesing , P. Dinaucourt , A. Djakonow , T. Djemil , A. Ebersoldt , T. Ebisuzaki , J. Eser , F. Fenu , S. Fernández-González , S. Ferrarese , G. Filippatos , W. Finch , C. Fornaro , M. Fouka , A. Franceschi , S. Franchini , C. Fuglesang , T. Fujii , M. Fukushima , P. Galeotti , E. García-Ortega , D. Gardiol , G. K. Garipov , E. Gascón , E. Gazda , J. Genci , A. Golzio , P. Gorodetzky , R. Gregg , A. Green , F. Guarino , C. Guépin , A. Guzmán , Y. Hachisu , A. Haungs , T. Heigbes , J. Hernández Carretero , L. Hulett , D. Ikeda , N. Inoue , S. Inoue , F. Isgrò , Y. Itow , T. Jammer , S. Jeong , J. Jochum , E. Joven , E. G. Judd , A. Jung , F. Kajino , T. Kajino , S. Kalli , I. Kaneko , M. Kasztelan , K. Katahira , K. Kawai , Y. Kawasaki , A. Kedadra , H. Khales , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , M. Kleifges , P. A. Klimov , I. Kreykenbohm , J. F. Krizmanic , K. Królik , V. Kungel , Y. Kurihara , A. Kusenko , E. Kuznetsov , H. Lahmar , F. Lakhdari , J. Licandro , L. López Campano , F. López Martínez , S. Mackovjak , M. Mahdi , D. Mandát , M. Manfrin , L. Marcelli , J. L. Marcos , W. Marszał , Y. Martín , O. Martinez , K. Mase , M. Mastafa , J. N. Matthews , N. Mebarki , G. Medina-Tanco , A. Menshikov , A. Merino , M. Mese , J. Meseguer , S. S. Meyer , J. Mimouni , H. Miyamoto , Y. Mizumoto , A. Monaco , J. A. Morales de los Ríos , J. M. Nachtman , S. Nagataki , S. Naitamor , T. Napolitano , A. Neronov , K. Nomoto , T. Nonaka , T. Ogawa , S. Ogio , H. Ohmori , A. V. Olinto , Y. Onel , G. Osteria , A. N. Otte , A. Pagliaro , W. Painter , M. I. Panasyuk , B. Panico , E. Parizot , I. H. Park , B. Pastircak , T. Paul , M. Pech , I. Pérez-Grande , F. Perfetto , T. Peter , P. Picozza , S. Pindado , L. W. Piotrowski , S. Piraino , Z. Plebaniak , A. Pollini , E. M. Popescu , R. Prevete , G. Prévôt , H. Prieto , M. Przybylak , G. Puehlhofer , M. Putis , P. Reardon , M. H. Reno , M. Reyes , M. Ricci , M. D. Rodríguez Frías , O. F. Romero Matamala , F. Ronga , M. D. Sabau , G. Saccá , H. Sagawa , Z. Sahnoune , A. Saito , N. Sakaki , H. Salazar , J. L. Sánchez , J. C. Sanchez Balanzar , A. Santangelo , A. Sanz-Andrés , O. A. Saprykin , F. Sarazin , M. Sato , A. Scagliola , T. Schanz , H. Schieler , P. Schovánek , V. Scotti , M. Serra , S. A. Sharakin , H. M. Shimizu , K. Shinozaki , J. F. Soriano , A. Sotgiu , I. Stan , I. Strharský , N. Sugiyama , D. Supanitsky , M. Suzuki , J. Szabelski , N. Tajima , T. Tajima , Y. Takahashi , M. Takeda , Y. Takizawa , M. C. Talai , Y. Tameda , C. Tenzer , S. B. Thomas , O. Tibolla , L. G. Tkachev , T. Tomida , N. Tone , S. Toscano , M. Traïche , Y. Tsunesada , K. Tsuno , S. Turriziani , Y. Uchihori , J. F. Valdés-Galicia , P. Vallania , L. Valore , G. Vankova-Kirilova , T. M. Venters , C. Vigorito , L. Villaseñor , B. Vlcek , P. von Ballmoos , M. Vrabel , S. Wada , J. Watanabe , J. Watts. , R. Weigand Muñoz , A. Weindl , L. Wiencke , M. Wille , J. Wilms , T. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , S. Yoshida , R. Young , I. S. Zgura , M. Yu. Zotov , A. Zuccaro Marchi