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The Local Interstellar Medium (LISM) is a unique environment that presents an opportunity to study general interstellar phenomena in great detail and in three dimensions. In particular, high resolution optical and ultraviolet spectroscopy…

Astrophysics · Physics 2007-05-23 Seth Redfield

This white paper recognizes gaps in observations that will, when addressed, much improve solar radiation hazard and geomagnetic storm forecasting. Radiation forecasting depends on observations of the entire "Solar Radiation Hemisphere" that…

Instrumentation and Methods for Astrophysics · Physics 2023-01-12 A. Posner , N. Arge , K. Cho , B. Heber , F. Effenberger , T. Y. Chen , S. Krucker , P. Kühl , O. Malandraki , Y. -D. Park , A. Pulkkinen , N. Raouafi , S. K. Solanki , O. C. StCyr , R. D. Strauss

The Alpha Magnetic Spectrometer (AMS-02) is a high energy particle physics experiment that will study cosmic rays in the $\sim 100 \mathrm{MeV}$ to $1 \mathrm{TeV}$ range and will be installed on the International Space Station (ISS) for at…

High Energy Physics - Experiment · Physics 2008-11-26 01 Collaboration

The use of eXtended Reality (XR) technologies in the space domain has increased significantly over the past few years as it can offer many advantages when simulating complex and challenging environments. Space agencies are currently using…

Human-Computer Interaction · Computer Science 2024-10-22 Florian Saling , Andrea Emanuele Maria Casini , Andreas Treuer , Martial Costantini , Leonie Bensch , Tommy Nilsson , Lionel Ferra

NASA's Artemis Mission aims to return astronauts to the Moon and establish a base at the lunar south pole. A key challenge is understanding the threat from micrometeoroid impacts, which are too small to monitor directly. Using NASA's…

In addition to the omnipresent Galactic Cosmic Rays (GCRs), sudden solar energetic particle (SEP) events present considerable health hazards for manned space missions. These events not only contribute to an increased long-term cancer risk,…

Low-frequency radio observatories are reaching unprecedented levels of sensitivity in an effort to detect the 21 cm signal from the Cosmic Dawn. High precision is needed because the expected signal is overwhelmed by foreground…

Instrumentation and Methods for Astrophysics · Physics 2022-03-14 Adam E. Lanman , Steven G. Murray , Daniel C. Jacobs

We present the basic elements and first results of an end-to-end simulation package whose purpose is to test the validity of the Space Interferometer Mission design. The fundamental simulation time step is one millisecond, with substructure…

Astrophysics · Physics 2009-11-10 David L. Meier , William M. Folkner

The X-ray Imaging and Spectroscopy Mission (XRISM), launched into low-Earth orbit in 2023, observes the reflection of solar flare X-rays in the Earth's atmosphere as a by-product of celestial observations. Using a $\sim$one-year data set…

The RADiation-hard Electron Monitor (RADEM) aboard the Jupiter Icy Moons Explorer (JUICE), launched on 14 April 2023, measures high-energy protons and electrons during the cruise phase and will continue throughout the nominal mission.…

Research-based active learning approaches are critical for the teaching and learning of undergraduate STEM majors. Course-based undergraduate research experiences (CUREs) are becoming more commonplace in traditional, in-person academic…

Physics Education · Physics 2024-05-27 Justin Hom , Jennifer Patience , Karen Knierman , Molly N. Simon , Ara Austin

The concern on human health is often overseen while wearable technologies attract exploding interests. Mainly due to the extreme proximity or a direct physical contact to the human skin, wearable communications devices are acknowledged to…

Signal Processing · Electrical Eng. & Systems 2019-12-12 Seungmo Kim , Yakub Sharif , Imtiaz Nasim

We evaluate the exposure during nadir observations with JEM-EUSO, the Extreme Universe Space Observatory, on-board the Japanese Experiment Module of the International Space Station. Designed as a mission to explore the extreme energy…

High Energy Astrophysical Phenomena · Physics 2013-05-14 J. H. Adams , S. Ahmad , J. -N. Albert , D. Allard , M. Ambrosio , L. Anchordoqui , A. Anzalone , Y. Arai , C. Aramo , K. Asano , M. Ave , P. Barrillon , T. Batsch , J. Bayer , T. Belenguer , R. Bellotti , A. A. Berlind , M. Bertaina , P. L. Biermann , S. Biktemerova , C. Blaksley , J. Blecki , S. Blin-Bondil , J. Bluemer , P. Bobik , M. Bogomilov , M. Bonamente , M. S. Briggs , S. Briz , A. Bruno , F. Cafagna , D. Campana , J-N. Capdevielle , R. Caruso , M. Casolino , C. Cassardo , G. Castellini , O. Catalano , A. Cellino , M. Chikawa , M. J. Christl , V. Connaughton , J. F. Cortes , H. J. Crawford , R. Cremonini , S. Csorna , J. C. D'Olivo , S. Dagoret-Campagne , A. J. de Castro , C. De Donato , C. de la Taille , L. del Peral , A. Dell'Oro , M. P. De Pascale , M. Di Martino , G. Distratis , M. Dupieux , A. Ebersoldt , T. Ebisuzaki , R. Engel , S. Falk , K. Fang , F. Fenu , I. Fernandez-Gomez , S. Ferrarese , A. Franceschi , J. Fujimoto , P. Galeotti , G. Garipov , J. Geary , U. G. Giaccari , G. Giraudo , M. Gonchar , C. Gonzalez Alvarado , P. Gorodetzky , F. Guarino , A. Guzman , Y. Hachisu , B. Harlov , A. Haungs , J. Hernandez Carretero , K. Higashide , T. Iguchi , H. Ikeda , N. Inoue , S. Inoue , A. Insolia , F. Isgrio , Y. Itow , E. Joven , E. G. Judd , A. Jung , F. Kajino , T. Kajino , I. Kaneko , Y. Karadzhov , J. Karczmarczyk , K. Katahira , K. Kawai , Y. Kawasaki , B. Keilhauer , B. A. Khrenov , Jeong-Sook Kim , Soon-Wook Kim , Sug-Whan Kim , M. Kleifges , P. A. Klimov , S. H. Ko , D. Kolev , I. Kreykenbohm , K. Kudela , Y. Kurihara , E. Kuznetsov , G. La Rosa , J. Lee , J. Licandro , H. Lim , F. Lopez , M. C. Maccarone , K. Mannheim , L. Marcelli , A. Marini , G. Martin-Chassard , O. Martinez , G. Masciantonio , K. Mase , R. Matev , A. Maurissen , G. Medina-Tanco , T. Mernik , H. Miyamoto , Y. Miyazaki , Y. Mizumoto , G. Modestino , D. Monnier-Ragaigne , J. A. Morales de los Rios , B. Mot , T. Murakami , M. Nagano , M. Nagata , S. Nagataki , T. Nakamura , J. W. Nam , S. Nam , K. Nam , T. Napolitano , D. Naumov , A. Neronov , K. Nomoto , T. Ogawa , H. Ohmori , A. V. Olinto , P. Orleanski , G. Osteria , N. Pacheco , M. I. Panasyuk , E. Parizot , I. H. Park , B. Pastircak , T. Patzak , T. Paul , C. Pennypacker , T. Peter , P. Picozza , A. Pollini , H. Prieto , P. Reardon , M. Reina , M. Reyes , M. Ricci , I. Rodriguez , M. D. Rodriguez Frias , F. Ronga , H. Rothkaehl , G. Roudil , I. Rusinov , M. Rybczynski , M. D. Sabau , G. Saez Cano , A. Saito , N. Sakaki , M. Sakata , H. Salazar , S. Sanchez , A. Santangelo , L. Santiago Cruz , M. Sanz Palomino , O. Saprykin , F. Sarazin , H. Sato , M. Sato , T. Schanz , H. Schieler , V. Scotti , M. Scuderi , A. Segreto , S. Selmane , D. Semikoz , M. Serra , S. Sharakin , T. Shibata , H. M. Shimizu , K. Shinozaki , T. Shirahama , G. Siemieniec-Ozieb , H. H. Silva Lopez , J. Sledd , K. Slominska , A. Sobey , T. Sugiyama , D. Supanitsky , M. Suzuki , B. Szabelska , J. Szabelski , F. Tajima , N. Tajima , T. Tajima , Y. Takahashi , H. Takami , M. Takeda , Y. Takizawa , C. Tenzer , O. Tibolla , L. Tkachev , T. Tomida , N. Tone , F. Trillaud , R. Tsenov , K. Tsuno , T. Tymieniecka , Y. Uchihori , O. Vaduvescu , J. F. Valdes-Galicia , P. Vallania , L. Valore , G. Vankova , C. Vigorito , L. Villasenor , P. von Ballmoos , S. Wada , J. Watanabe , S. Watanabe , J. Watts , M. Weber , T. J. Weiler , T. Wibig , L. Wiencke , M. Wille , J. Wilms , Z. Wlodarczyk , T. Yamamoto , Y. Yamamoto , J. Yang , H. Yano , I. V. Yashin , D. Yonetoku , K. Yoshida , S. Yoshida , R. Young , A. Zamora , A. Zuccaro Marchi

The Am $5d$-$5f$ resonant inelastic x-ray scattering (RIXS) data of americium sesquioxide were measured at incident photon energies throughout the Am $O_{4,5}$ edges. The experiment was supported by calculations using several model…

Strongly Correlated Electrons · Physics 2023-09-06 Sergei M. Butorin , David K. Shuh

The Alpha Magnetic Spectrometer (AMS), whose final version AMS-02 is to be installed on the International Space Station (ISS) for at least 3 years, is a detector designed to measure charged cosmic ray spectra with energies up to the TeV…

Astrophysics · Physics 2008-01-22 Luísa Arruda , Fernando Barão , Rui Pereira

A measurement of the dipole anisotropy in galactic coordinates for different charged cosmic rays has been performed with the Alpha Magnetic Spectrometer (AMS) onboard the International Space Station (ISS). Results are presented for the…

High Energy Astrophysical Phenomena · Physics 2019-10-16 M. Molero , J. Casaus , C. Mana , M. A. Velasco , I. Gebauer , M. Graziani , M. Gervasi , G. La Vacca , P. G. Rancoita

The expected physics and astrophysics capabilities of the AMS experiment on board the International Space Station are briefly reviewed : high statistics study of cosmic rays in a wide range of energies, search for primordial antimatter,…

Astrophysics · Physics 2007-05-23 Aurelien Barrau , AMS collaboration

The unprecedented quality of the data collected by the AMS-02 experiment onboard the International Space Station allowed us to address subtle questions concerning the origin and propagation of cosmic rays. Here we discuss the implications…

High Energy Astrophysical Phenomena · Physics 2019-06-05 Carmelo Evoli , Roberto Aloisio , Pasquale Blasi

The past three decades have seen prodigious advances in astronomy and astrophysics. Beginning with the exploration of our solar system and continuing through the pioneering Explorers and Great Observatories of today, NASA missions have made…

The ESA-Ariel mission will include a tier dedicated to exoplanet phase curves corresponding to ~10% of the science time. We present here the current observing strategy for studying exoplanet phase curves with Ariel. We define science…