Results 61 to 70 of about 23,959 (174)
A low cost scheme for high precision dual-wavelength laser metrology
, 2013 A novel method capable of delivering relative optical path length metrology
with nanometer precision is demonstrated. Unlike conventional dual-wavelength
metrology which employs heterodyne detection, the method developed in this work
utilizes direct ...Ireland, Michael J., Kok, Yitping, Robertson, J. Gordon, Tango, William J., Tuthill, Peter G., Warrington, Benjamin A. +5 morecore +1 more sourceLongitudinal Variability of Pre‐Midnight Equatorial Plasma Bubbles Under Disturbed Geomagnetic Conditions
Journal of Geophysical Research: Space Physics, Volume 131, Issue 1, January 2026.Abstract
Equatorial plasma bubbles (EPBs) pose significant challenges to trans‐ionospheric radio communication and navigation systems. Because of their disruptive effects, evaluating and predicting them is key for the development of space systems. The influence of geomagnetic activity on EPBs remains unclear, partly due to limited low‐latitude neutral ...Gilda de Lourdes González, Thomas J. Immel, Yen‐Jung Wu, L. Claire Gasque, Brian J. Harding, Colin Triplett, Cesar E. Valladares +6 morewiley +1 more sourceAstronomical photonics in the context of infrared interferometry and
high-resolution spectroscopy
, 2016 We review the potential of Astrophotonics, a relatively young field at the
interface between photonics and astronomical instrumentation, for
spectro-interferometry.Aggarwal, Berio, Coudé du Foresto, Diener, Eisenhauer, Errmann, Froehly, Guieu, Haynes, Jorden, Labadie, Labeye, Lhomé, Lindley, Martin, Martín, Norris, Russell, Tepper +18 morecore +3 more sourcesPerformance of the Imaging Fourier Transform Spectrometer with
Photoconductive Detector Arrays: An Application for the AKARI Far-Infrared
Instrument
, 2008 We have developed an imaging Fourier transform spectrometer (FTS) for
space-based far-infrared astronomical observations. The FTS employs a newly
developed photoconductive detector arrays with a capacitive trans-impedance
amplifier, which makes the FTS a DOI, Yasuo, KANEDA, Hidehiro, KAWADA, Mitsunobu, MATSUO, Hiroshi, MATSUURA, Shuji, MURAKAMI, Noriko, NAKAGAWA, Takao, OKADA, Yoko, OOTSUBO, Takafumi, SHIBAI, Hiroshi, SHIRAHATA, Mai, TAKAHASHI, Hidenori, YASUDA, Akiko, 中川, 貴雄, 土井, 靖生, 大坪, 貴文, 安田, 晃子, 岡田, 陽子, 川田, 光伸, 村上, 紀子, 松尾, 宏, 松浦, 周二, 白旗, 麻衣, 芝井, 広, 金田, 英宏, 高橋, 英則 +25 morecore +1 more sourceComparative Analysis of Ionospheric Responses to Ultra‐Fast Kelvin Waves With Wavenumbers 1, 2, and 3
Space Weather, Volume 24, Issue 1, January 2026.Abstract
We employed zonal wind data from Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics Doppler Interferometer, equatorial electrojet (EEJ) measurements from Jicamarca (12°S, 77°W), and global ionospheric total electron content (TEC) maps to investigate the effects of ultra‐fast Kelvin waves (UFKW) with zonal wavenumbers 2 and 3 ...Ruidi Sun, Sheng‐Yang Gu, Yusong Qin, Hui Huang, Shuyue Zhao, Dini Gong, Min Jiang +6 morewiley +1 more sourceWaveform modelling for the Laser Interferometer Space Antenna
Living Reviews in RelativityLISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay, Pau Amaro Seoane, Andrea Antonelli, Josu C. Aurrekoetxea, Leor Barack, Enrico Barausse, Robert Benkel, Laura Bernard, Sebastiano Bernuzzi, Emanuele Berti, Matteo Bonetti, Béatrice Bonga, Gabriele Bozzola, Richard Brito, Alessandra Buonanno, Alejandro Cárdenas-Avendaño, Marc Casals, David F. Chernoff, Alvin J. K. Chua, Katy Clough, Marta Colleoni, Geoffrey Compère, Mekhi Dhesi, Adrien Druart, Leanne Durkan, Guillaume Faye, Deborah Ferguson, Scott E. Field, William E. Gabella, Juan García-Bellido, Miguel Gracia-Linares, Davide Gerosa, Stephen R. Green, Maria Haney, Mark Hannam, Anna Heffernan, Tanja Hinderer, Thomas Helfer, Scott A. Hughes, Sascha Husa, Soichiro Isoyama, Michael L. Katz, Chris Kavanagh, Gaurav Khanna, Larry E. Kidder, Valeriya Korol, Lorenzo Küchler, Pablo Laguna, François Larrouturou, Alexandre Le Tiec, Benjamin Leather, Eugene A. Lim, Hyun Lim, Tyson B. Littenberg, Oliver Long, Carlos O. Lousto, Geoffrey Lovelace, Georgios Lukes-Gerakopoulos, Philip Lynch, Rodrigo P. Macedo, Charalampos Markakis, Elisa Maggio, Ilya Mandel, Andrea Maselli, Josh Mathews, Pierre Mourier, David Neilsen, Alessandro Nagar, David A. Nichols, Jan Novák, Maria Okounkova, Richard O’Shaughnessy, Naritaka Oshita, Conor O’Toole, Zhen Pan, Paolo Pani, George Pappas, Vasileios Paschalidis, Harald P. Pfeiffer, Lorenzo Pompili, Adam Pound, Geraint Pratten, Hannes R. Rüter, Milton Ruiz, Zeyd Sam, Laura Sberna, Stuart L. Shapiro, Deirdre M. Shoemaker, Carlos F. Sopuerta, Andrew Spiers, Hari Sundar, Nicola Tamanini, Jonathan E. Thompson, Alexandre Toubiana, Antonios Tsokaros, Samuel D. Upton, Maarten van de Meent, Daniele Vernieri, Jeremy M. Wachter, Niels Warburton, Barry Wardell, Helvi Witek, Vojtěch Witzany, Huan Yang, Miguel Zilhão, Angelica Albertini, K. G. Arun, Miguel Bezares, Alexander Bonilla, Christian Chapman-Bird, Bradley Cownden, Kevin Cunningham, Chris Devitt, Sam Dolan, Francisco Duque, Conor Dyson, Chris L. Fryer, Jonathan R. Gair, Bruno Giacomazzo, Priti Gupta, Wen-Biao Han, Roland Haas, Eric W. Hirschmann, E. A. Huerta, Philippe Jetzer, Bernard Kelly, Mohammed Khalil, Jack Lewis, Nicole Lloyd-Ronning, Sylvain Marsat, Germano Nardini, Jakob Neef, Adrian Ottewill, Christiana Pantelidou, Gabriel Andres Piovano, Jaime Redondo-Yuste, Laura Sagunski, Leo C. Stein, Viktor Skoupý, Ulrich Sperhake, Lorenzo Speri, Thomas F. M. Spieksma, Chris Stevens, David Trestini, Alex Vañó-Viñuales +146 moredoaj +1 more sourceLOOC UP: Locating and observing optical counterparts to gravitational
wave bursts
, 2008 Gravitational wave (GW) bursts (short duration signals) are expected to be
associated with highly energetic astrophysical processes. With such high
energies present, it is likely these astrophysical events will have signatures
in the EM spectrum as well ..., , , Abbott B, Abbott B, Acernese F (for the Virgo Collaboration), Adhikari R Fritschel P Waldman S, Chatterji S, Chatterji S, David C Murphy, Jennifer Piscionere, Jonah Kanner, Kahya E O, Kochanek C S, Kopparapu R K, Li L, Markowitz J Zanolin M Cadonati L Katsavounidis E, McNabb J W C, Molly Reed, Müller E, Peter Shawhan, Richardson D, Sadowski A, Stubbs C W, Sylvestre J, Szabolcs Márka, Tracy L Huard +26 morecore +1 more sourceJAXA curation for Bennu samples returned by the NASA's OSIRIS‐REx mission
Meteoritics &Planetary Science, Volume 61, Issue 1, Page 182-207, January 2026.Abstract
NASA's OSIRIS‐REx mission successfully collected and returned ~121.6 g of bulk samples from the B‐type, near‐Earth asteroid (101955) Bennu to Earth in September 2023. Upon returning to Earth, the samples were transported to the NASA Johnson Space Center where most of the samples have been stored and processed.Rui Tahara, Kentaro Hatakeda, Masahiro Nishimura, Kasumi Yogata, Ryota Fukai, Akiko Miyazaki, Toru Yada, Yuma Enokido, Masanao Abe, Seiya Kawasaki, Ryosuke Sakurai, Tatsuaki Okada, Cedric Pilorget, Jean‐Pierre Bibring, Vincent Hamm, Lionel Lourit, Damien Loizeau, Lucie Riu, Koki Yumoto, Yuichiro Cho, Seiji Sugita, Shumpei Nakahara, Shoki Mori, Yuta Aikyo, Shingo Kameda, Roger Stabbins, Yuta Shimizu, Hideaki Miyamoto, Yuya Hitomi, Arisa Nakano, Kana Nagashima, Haruna Sugahara, Shino Suzuki, Shunta Kimura, Tomohiro Usui +34 morewiley +1 more source