波霎 的英文怎麼說

中文拼音 [shà]
波霎 英文
pulsar
  • : Ⅰ名詞1 (波浪) wave 2 [物理學] (振動傳播的過程) wave 3 (意外變化) an unexpected turn of even...
  • : 名詞(短時間; 一會兒) a very short time; moment; instant
  1. Yet the march 1979 burster, with an apparent rotation period of eight seconds, was spinning much more slowly than any radio pulsar then known

    但1979年3月那次的爆炸源,看起來卻有八秒的周期,自轉速率要比當時所知的任何波霎還要慢得多。
  2. From this, most young radio pulsars are inferred to have magnetic fields between 1012 and 1013 gauss

    從這個論點來推斷,大部份年輕的無線電波霎應具有介於1012 ~ 1013高斯的磁場。
  3. One ramification of our calculations is that radio pulsars are neutron stars in which the large - scale dynamo has failed to operate

    從我們的計算中,還可以附帶得到一點:無線電波霎正是無法形成大尺度發電機的中子星。
  4. The spin - down rate has been measured for almost every radio pulsar, and theory indicates that it depends on the strength of the star ' s magnetic field

    這種自轉變慢的速率,幾乎每一顆無線電波霎都量得到,而理論指出,此速率和星體的磁場強度有關。
  5. If the moving fluid in a newborn neutron star also transfers a tenth of its kinetic energy to the magnetic field, then the field would grow stronger than 1015 gauss, which is more than 1, 000 times as strong as the fields of most radio pulsars

    如果在新生中子星里的流體,也把10 %的動能轉變成磁場的話,磁場強度會上漲到超過1015高斯,這是大多數無線電波霎所帶磁場強度的1000倍以上。
  6. Topics include : planets, planet formation ; stars, the sun, " normal " stars, star formation ; stellar evolution, supernovae, compact objects ( white dwarfs, neutron stars, and black holes ), plusars, binary x - ray sources ; star clusters, globular and open clusters ; interstellar medium, gas, dust, magnetic fields, cosmic rays ; distance ladder ; galaxies, normal and active galaxies, jets ; gravitational lensing ; large scaling structure ; newtonian cosmology, dynamical expansion and thermal history of the universe ; cosmic microwave background radiation ; big - bang nucleosynthesis

    課程的主題包含了:行星、行星形成;恆星、太陽、正常的恆星、恆星形成;恆星演化、超新星、緻密天體(白矮星、中子星及黑洞) 、波霎、雙x -射線源;星團、球狀及疏散星團;星際介質、氣體、塵埃、磁場、宇宙射線;距離階梯;星系、正常及活躍星系、噴流;重力透鏡;大尺度結構;牛頓宇宙學、宇宙的動力膨脹及溫度發展歷史;宇宙背景微輻射;大霹靂核合成。
  7. Perhaps the most famous pulsar lies within the crab nebula, the remnant of a supernova explosion that was observed in 1054

    最有名的波霎,或許要算是蟹狀星雲里頭的那顆了,這片星雲是1054年觀測到的超新星爆炸的殘骸。
  8. Tai hang road, leighton road, sharp street east, percival street south of hennessy road, caroline hill road, link road, stadium path, cotton path, eastern hospital road, eastern hospital road service road, broadwood road, southbound wong nai chung gap road, southbound stubbs road flyover, aberdeen reservoir road and yue kwong road

    大坑道、禮頓道、東街、軒尼詩道以南的斯富街、加路連山道、連道、大球場徑、棉花路、東院道、東院道支路、樂活道、黃泥涌峽道南行、司徒拔道天橋南行、香港仔水塘道及漁光道。
  9. Rs route hr36 on journeys to ap lei chau will be diverted via percival street, sharp street east, canal road east, canal road west, canal road flyover, victoria park road, causeway bay flyover, gloucester road service road, canal road flyover and aberdeen tunnel ; and

    洲將改經斯富街東街堅拿道東堅拿道西堅拿道天橋維園道天橋告士打道西行線堅拿道天橋及香港仔隧道及
  10. If the core magnetic field started with sufficient strength, this compression could explain pulsar magnetism

    要是一開始的核心磁場夠強,星體塌縮的確可以解釋波霎的磁性。
  11. In the case of the crab pulsar, the newborn neutron star rotated once every 20 milliseconds, much slower than the rate of convection, so the dynamo never got going

    以蟹狀星雲中的波霎來說,新生的中子星每20毫秒自轉一周,比對流的速率要慢得多,因此它的發電機從來就沒有啟動過。
  12. The pulsar rotates once every 33 milliseconds and is currently slowing at a rate of about 1. 3 millisecond every century

    波霎每33毫秒自轉一周,其周期目前正以每世紀1 . 3毫秒的速率變慢。
分享友人