åœ°è¡¨æ¸©åº¦ä¸Žå‘å°„çŽ‡æ˜¯åœ°è¡¨â€”å¤§æ°”ç³»ç»Ÿé•¿æ³¢è¾å°„å’Œæ½œçƒ­é€šé‡äº¤æ¢çš„ç›´æŽ¥é©±åŠ¨åŠ›ï¼Œæ˜¯æè¿°åŒºåŸŸå’Œå ¨çƒå°ºåº¦ä¸Šåœ°è¡¨èƒ½é‡å¹³è¡¡ä¸Žæ°´å¹³è¡¡çš„é‡è¦å‚æ•°ï¼Œå ¶æ—¶ç©ºå˜åŒ–ä¿¡æ¯åœ¨æ°”è±¡é¢„æµ‹ã€æ°”å€™å˜åŒ–ã€æ°´å¾ªçŽ¯ã€åœ°è´¨å‹˜æŽ¢ã€å†œæž—ç›‘æµ‹å’ŒåŸŽå¸‚çƒ­çŽ¯å¢ƒç­‰è¯¸å¤šé¢†åŸŸå ·æœ‰å¹¿æ³›çš„åº”ç”¨ã€‚çƒ­çº¢å¤–é¥æ„Ÿä½œä¸ºå½“å‰èŽ·å–åŒºåŸŸæˆ–å ¨çƒå°ºåº¦ä¸Šåœ°è¡¨æ...

åœ°è¡¨å®žé™ è’¸æ•£å‘æ˜¯è”ç³»é™†è¡¨æ°´å¾ªçŽ¯ã€èƒ½é‡å¹³è¡¡å’Œç¢³æ”¶æ”¯ç­‰ç‰©ç†è¿‡ç¨‹çš„é‡è¦ç”Ÿæ€æ°´æ–‡å˜é‡ï¼ŒåŒæ—¶ä¹Ÿæ˜¯ç›®å‰æ°´å¾ªçŽ¯ç ”ç©¶ä¸­çš„è–„å¼±ç‚¹ï¼Œå®šé‡åŒ–åœŸå£¤æ°´åˆ†å¯¹è’¸æ•£å‘çš„èƒè¿«ä½œç”¨æ˜¯ä¼°ç®—åœ°è¡¨è’¸æ•£å‘çš„ä¸€ä¸ªå ³é”®è¿‡ç¨‹å’Œéš¾ç‚¹ã€‚æœ¬ç ”ç©¶åŸºäºŽ2018å¹´9月闪电河流域水循环与能量平衡遥感综合试验星—机—地联合观测数据，采ç”...

è½¦è½½ç§»åŠ¨æµ‹é‡ç³»ç»Ÿå¯é‡‡é›†é«˜ç²¾åº¦é“è·¯ä¸‰ç»´ç‚¹äº‘æ•°æ®ï¼Œä¸ºé“è·¯è¾¹ç•Œè‡ªåŠ¨åŒ–æå–æä¾›äº†æ”¯æ’‘ã€‚ä¸ºè§£å†³è½¦è½½æ¿€å ‰ç‚¹äº‘ä¸­åŸŽå¸‚é“è·¯è¾¹ç•Œç‚¹äº‘æå–å›°éš¾é—®é¢˜ï¼Œæœ¬æ–‡å¼•å ¥å±€éƒ¨äºŒå€¼æ¨¡å¼LBP（Local Binary Pattern），针对各类城市道路边界特征，设计了高度LBP、高程离散度LBP和空间形状LBP 3ç§æ”¹è¿›ç®—å­ï¼›æž„å»ºå¤šå ƒLBP特征语义...

é’ˆå¯¹å•è½´æŠ›å ‰æœºé¢å½¢æŽ§åˆ¶éš¾åº¦å¤§ã€è¾ƒå¤šä¾èµ–äººå·¥ç»éªŒï¼Œæ— æ³•æ»¡è¶³å ‰å­¦å ƒä»¶æ¿€å¢žçš„æ•°é‡å’Œç²¾åº¦éœ€æ±‚çš„é—®é¢˜ï¼Œæå‡ºç ”åˆ¶ä¸€ç§æ–°åž‹è¶ ç²¾å¯†çŽ¯å½¢æŠ›å ‰æœºåºŠã€‚é¦–å ˆå¼•å ¥æŠ›å ‰ç›˜è·³åŠ¨ä¸ºå˜é‡æž„å»ºåŸºäºŽPrestonå ¬å¼å’Œèµ«å ¹æŽ¥è§¦ç†è®ºçš„ææ–™åŽ»é™¤æ¨¡åž‹ï¼›æ¨¡åž‹ä»¿çœŸåˆ†æžè¡¨æ˜ŽæŠ›å ‰ç›˜è·³åŠ¨è¯¯å·®å˜åŒ–ä¼šå¯¼è‡´ææ–™ä¸å‡åŒ€åŽ»é™¤ï¼Œè€Œä¸»è½´è·³åŠ¨...

Using the University of California Berkeley Infrared Spatial Interferometer with a radio frequency (RF) Ðlter bank, the Ðrst interferometric observations of mid-infrared molecular absorption features of ammonia and silane with very high spectral resolution (j/*jD 105) were made. Under the 3 4 assumptions of spherical symmetry and uniform outÑow, these new data permitted the molecular stratiÐcat...

We use recent data obtained by three (OSSE, BATSE, and COMPTEL) of four instruments on board the Compton Gamma Ray Observatory (CGRO) to construct a model of Cyg X-1 that describes its emission in a broad energy range, from soft X-rays to MeV c-rays, self-consistently. The c-ray emission is interpreted to be the result of Comptonization, bremsstrahlung, and positron annihilation in a hot, optic...

We analyze archival ROSAT HRI, ROSAT PSPC, and ASCA data of the X-rayÈfaint early-type galaxy NGC 4697. The joint ROSAT PSPC]ASCA spectrum is Ðtted by a two-component thermal model, a MEKAL model with keV with low metallicity and a bremsstrahlung kT MEKAL \ 0.26 ~0.03 `0.04 model with keV. A similar model was found to Ðt the spectra of another faint earlykT BREM \ 5.2 ~1.6 `3.0 type galaxy (NGC...

é«˜åˆ†è¾¨çŽ‡é¥æ„Ÿå½±åƒä¸­è€•åœ°ç‰¹å¾å¤æ‚ï¼Œäººå·¥ç›®è§†è§£è¯‘å’Œä¼ ç»Ÿçš„é¥æ„Ÿå½±åƒåˆ†ç±»æ–¹æ³•æå–èƒ½åŠ›æœ‰é™ï¼Œæ— æ³•å®žçŽ°å¤§èŒƒå›´çš„è‡ªåŠ¨åŒ–é«˜ç²¾åº¦è€•åœ°æå–ã€‚æ·±åº¦å­¦ä¹ æŠ€æœ¯å› å ·æœ‰è¾ƒå¼ºçš„åœ°ç‰©è¡¨è¾¾èƒ½åŠ›ï¼Œåœ¨é¥æ„Ÿå½±åƒä¿¡æ¯è‡ªåŠ¨æå–æ–¹é¢è¡¨çŽ°å‡ºäº†ä¼˜è¶Šçš„æ€§èƒ½ï¼Œä¸ºå¤§èŒƒå›´è€•åœ°çš„ç²¾ç»†åŒ–è‡ªåŠ¨æå–æä¾›äº†æ–°çš„æ€è·¯ã€‚æŽ¢ç©¶ä¸åŒå ¸åž‹ç½‘ç»œæ...

é‡‘å±žå¤åŒ–ç‰©é’™é’›çŸ¿å‘å ‰äºŒæžç®¡ï¼ˆPerovskite light⁃emitting diodes， Pero⁃LEDsï¼‰å™¨ä»¶ç»“æž„ä¸­ï¼Œç©ºç©´ä¼ è¾“å±‚ï¼ˆHTL）是影响Pero⁃LEDsæ•ˆçŽ‡çš„å ³é”®æ€§å› ç´ ä¹‹ä¸€ã€‚ç”±äºŽé†‹é ¸é’´ï¼ˆCo（OAc）2ï¼‰è–„è†œå ·æœ‰ä¼˜å¼‚çš„å ‰ç”µç‰¹æ€§ï¼Œæ‰€ä»¥é€‰å ¶ä½œä¸ºç»¿å ‰Pero⁃LEDs的HTLã€‚ç„¶è€Œï¼Œçº¯çš„é’´åŸºåº•è–„è†œå­˜åœ¨ä¼ è¾“è½½æµå­èƒ½åŠ›è¾ƒå·®ã€è–„è†œç²—ç³™åº¦è¾ƒå¤§ç­‰é—®é¢...

å«æ˜Ÿé¥æ„Ÿè½½è·åœ¨è½¨è¾å°„å®šæ ‡éœ€è¦é«˜ç¨³å®šã€é«˜å¯é ã€å¯è¿½æº¯çš„è¾å°„å®šæ ‡æºæ”¯æŒã€‚å°†è¾å°„åŸºå‡†æ¬è‡³ç©ºé—´å¹³å°ï¼Œåˆ©ç”¨åŒæ­¥å¯¹åœ°è§‚æµ‹çš„æ–¹å¼å°†åŸºå‡†ä¼ é€’è‡³å«æ˜Ÿè½½è·ï¼Œå·²æˆä¸ºæœªæ¥æå‡åœ¨è½¨è¾å°„å®šæ ‡ç²¾åº¦çš„å¯è¡Œæ–¹å¼ä¹‹ä¸€ã€‚ä¸´è¿‘ç©ºé—´é«˜åº¦ä¸Šå¯èŽ·å¾—ä¸Žå«æ˜Ÿç›¸æŽ¥è¿‘çš„è§‚æµ‹ï¼ŒåŒæ—¶ï¼Œä»¥é«˜ç©ºç§‘å­¦æ°”çƒä¸ºä»£è¡¨çš„ä¸´è¿‘ç©ºé—´æµ®ç©ºå™¨è...