The remnant nebular gas pervades the interplanetary space . 星云的殘余氣體充斥星際空間。
Comprehensive studies on magnetic clouds in interplanetary space and their associated events 行星際磁云及其相關(guān)事件的綜合研究
The solar wind has its own magnetic field , which travels with the outflowing plasma into interplanetary space 太陽風(fēng)有它自己的磁場,這個磁場會隨著外流的太陽風(fēng)電漿一起流入星際空間。
The field that space environment contain is high - layer atmosphere , ionosphere , magnetic layer , interplanetary space and even sun 涵蓋的區(qū)域包括地球高層大氣、電離層、磁層、行星際空間直至太陽。
A very small fraction of the sun ' s light and heat is emitted in such directions that after passing unhindered through interplanetary space , it hits the earth 只有很小一部分太陽的光和熱由此方向釋放出來,并且未被阻擋,穿越星空,來到地球。
We are investigating the possibility of a commercial venture , where a solar sail would conduct station - keeping at points in interplanetary space that are useful for monitoring in the solar system 我們研究了一種商業(yè)風(fēng)險的可行性,就是太陽帆能定點(diǎn)保持在太陽系內(nèi)的某處,這對監(jiān)測太陽系很有用。
Such experiments , which would put the biological materials within simulated meteoritic materials and expose them to the environment of interplanetary space , could be conducted on the surface of the moon 這類實(shí)驗(yàn)要將生物體置入仿造的隕石物質(zhì)內(nèi),并且暴露于行星際空間的環(huán)境,月球表面可充當(dāng)試驗(yàn)場。
When structures of cmes are traveling in the interplanetary space and towards to the earth , some galactic cosmic ray ( ocr ) may penetrate through the structures or be refracted by them before reaching the earth ' s surface 當(dāng)行星際空間有cme朝向地球運(yùn)動時,一部分銀河宇宙線在穿過行星際空間時要穿過cme或遇到cme而折射到達(dá)地面,銀河宇宙線的速度很高,它們比cme要提前到達(dá)地面。
Solar wind flows out from the corona the sun s outer atmosphere into interplanetary space at speed of between 300 and 900 km per second . it causes fluctuation to the earth s magnetic field , which we call magnetic storm . such event will cause deflection of compass needles 而太陽風(fēng)則以每秒300至900千米的速度由日冕太陽外大氣層向外拋射,進(jìn)入行星際空間,對地球磁場造成擾動而產(chǎn)生磁暴,導(dǎo)致指南針指針偏移,嚴(yán)重的話更會導(dǎo)致電力受阻和電話線路中斷。
More and more researches have shown that most of the intense geomagnetic storms are caused by fast coronal mass ejections in interplanetary space ( icmes ) . though the ace satellite can provide solar wind data in almost real time for prediction of geomagnetic storms , the time interval is too short ( shorter than 30 - min ) for effective predictions of major geomagnetic storms 位于拉格朗日點(diǎn)的ace衛(wèi)星可以提供近實(shí)時的太陽風(fēng)數(shù)據(jù),但依據(jù)ace衛(wèi)星太陽風(fēng)數(shù)據(jù)進(jìn)行地磁暴預(yù)報,時間的提前量非常有限,對于大地磁暴,這個時間提前量往往不超過30分鐘,這樣的時間提前量對于實(shí)際應(yīng)用來說,是不能令人滿意的。