贵州台江下、中寒武统界线层型候选剖面碳同位素研究     

郭庆军  刘丛强  Harald Strauss  赵元龙  朱立军  皮道会  袁金良 《矿物学报》2006,26(3):303-311

在扬子地台贵州台江八郎下、中寒武统界线剖面界线附近,碳酸盐岩和干酪根碳同位素组成有规律变化。1δ3Cker(PDB)值在-33.4‰和-26.5‰间漂移与1δ3Ccarb(PDB)值在-2.7‰和 3.1‰间变化,反映了当时海水的碳同位素组成。无机和有机碳同位素组成之差的Δδ值,沿剖面不断变小,指示剖面上部样品可能受到热扰动和成岩后期作用影响。碳同位素规律的变化,反映了最初的沉积信息,特别是有机质埋藏量的变化,这些变化与早-中寒武世环境变化和生物组合差异有关。  相似文献   

Scientific detector workshop 2022 on-sky performance verification of near-infrared e−APD technology for wavefront sensing and demonstration of e−APD pixel performance to improve the sensitivity of large science focal planes     

Gert Finger  Frank Eisenhauer  Reinhard Genzel  Christopher Mandla  Ian Baker  Domingo Alvarez  Antonio Amorim  Wolfgang Brandner  Christophe Dupuy  Casey Deen  Derek Ives  Leander Mehrgan  Manfred Meyer  Karin Perraut  Guy Perrin  Jörg Stegmeier  Christian Straubmeier  Harald J. Weller  Vincent Isgar 《Astronomische Nachrichten》2023,344(8-9):e20230069

Near-infrared adaptive optics as well as fringe tracking for coherent beam combination in optical interferometry require the development of high-speed sensors. Because of the high speed, a large analog bandwidth is required. The short exposure times result in small signal levels which require noiseless detection. Both requirements cannot be met by state-of-the-art conventional CMOS technology of near-infrared arrays as has been attempted previously. A total of five near-infrared SAPHIRA 320 × 256 pixel HgCdTe e⁻APD arrays have been deployed in the wavefront sensors and in the fringe tracker of the VLTI instrument GRAVITY. The current limiting magnitude for coherent exposures with GRAVITY is m_k = 19, which is made possible with ADP technology. New avalanche photo-diode array (APD) developments since GRAVITY include the extension of the spectral sensitivity to the wavelength range from 0.8 to 2.5 μm. After GRAVITY a larger format array with 512 × 512 pixels has been developed for both AO applications at the ELT and for long integration times. Since dark currents of <10⁻³ e⁻/s have been demonstrated with 1Kx1K e⁻APD arrays and 2Kx2K e⁻APD arrays have already been developed, the possibilities and adaptations of e⁻APD technology to provide noiseless large-format science-grade arrays for long integration times are also discussed.  相似文献